ANS-075 AMSAT News Service Bulletins

ANS-075, March 16, 2025

In this edition:

* Amateur Satellites Finally Launch After Delays
* NASA’s SPHEREx, PUNCH Missions Launch
* ISS Changes Crew for Expedition 73
* Changes to AMSAT-NA TLE Distribution
* ARISS News
* Upcoming Satellite Operations
* AMSAT Ambassador Activities
* Satellite Shorts From All Over

The AMSAT News Service bulletins are a free, weekly news and information service of AMSAT, the Radio Amateur Satellite Corporation. ANS publishes news related to Amateur Radio in Space including reports on the activities of a worldwide group of Amateur Radio operators who share an active interest in designing, building, launching and communicating through analog and digital Amateur Radio satellites.

The news feed on http://www.amsat.org publishes news of Amateur Radio in Space as soon as our volunteers can post it.

Please send any amateur satellite news or reports to: ans-editor [at] amsat.org

Sign up for free e-mail delivery of the AMSAT News Service Bulletins via the ANS List; to join this list see: https://mailman.amsat.org/postorius/lists/ans.amsat.org/

Amateur Satellites Finally Launch After Delays

After delaying the launch of the mission a (highly unusual) seven times — it was originally slated to take to the skies on Feb. 27 — a SpaceX Falcon 9 rocket finally carried the 13th Rideshare to orbit on Saturday, March 15. The launch carried 74 small satellites to sun-sychronous orbit (SSO), lifting off from Vandenberg Space Force Base, California at 06:43 UTC (11:43 p.m. on March 14 local California time).


A SpaceX Falcon 9 rocket launches the Transporter 13 rideshare mission from Vandenberg Space Force Base in California on March 15, 2025. (Image credit: SpaceX)

Among the satellites aboard is HADES-ICM 1.5 PocketQube satellite main mission is to act as a FM voice repeater. It can also repeat FSK derived modes like FT-4 and FT-8. It has the same functionalities as in HADES-R (SO-124). FM and Digital modes repeater with Uplink on 145.875 MHz and Downlink on 436.666 MHz. It also carries the same experiment for SMART-IR/Manchester University. The repeater will not be active until all the checks have been performed on the satellite. This can take several weeks.

A group of satellites labeled as “TEVEL2” are on the launch manifest for the SpaceX Transporter 13 mission. Designated as TEVEL2-1 through TEVE2-9, they are all listed as having a downlink frequency of 436.400 MHz, and are expected to be activated in rotation, much in the same way as the previous constellation of TEVEL satellites, which have now all decayed from orbit.

A French cubesat named UVSQ-Sat NG — or “Next Generation” is also on the launch manifest. This satellite appears to have capabilities for amateur operation, however no such operation has been coordinated or announced.

See AMSAT News Service bulletins 061 for more details on all of these satellites.

[ANS thanks Space.com and AMSAT-EA for the above information]


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NASA’s SPHEREx, PUNCH Missions Launch

NASA’s SPHEREx and PUNCH missions were launched together on a SpaceX Falcon 9 rocket that lifted off from Vandenberg Space Force Base, California, on Tuesday evening, March 11 (early March 12 UTC). The launch had been delayed one day due to unfavorable weather at the launch site and an issue with one of the spacecraft.

SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) will then collect data on more than 450 million galaxies along with more than 100 million stars in the Milky Way in order to explore the origins of the universe, contributing to NASA Science’s key goals to discover the secrets of the universe and search for life elsewhere.


NASA’s SPHEREx mission will operate in low Earth orbit, detecting hundreds of millions of stars and galaxies and creating the first all-sky spectroscopic survey in the near-infrared. This artist’s concept shows the spacecraft and its distinctive conical photon shields, which protect SPHEREx’s telescope from infrared light and heat from the Sun and Earth. (Graphic: NASA/JPL-Caltech)

The mission’s 3D all-sky map will help scientists answer big-picture questions about the universe. The mission will investigate a cosmic phenomenon called inflation that caused the universe to expand rapidly for a fraction of a second after the big bang, measure the collective glow created by galaxies near and far, including hidden galaxies that have not been individually observed, and search the Milky Way galaxy for hidden reservoirs of water, carbon dioxide, and other essential ingredients for life.

The SPHEREx mission’s ability to scan large sections of the sky quickly and gather data on millions of objects complements the work of more targeted telescopes, like NASA’s Hubble and James Webb, and the observatory’s data will be freely available to scientists around the world, providing a new encyclopedia of information about hundreds of millions of cosmic objects.

Along for the ride was a second mission, PUNCH (Polarimeter to Unify the Corona and Heliosphere), a mission consisting of four satellites operating in concert. These small sats will observe the Sun’s corona as it transitions into the solar wind, supporting NASA Science’s key goals by creating a broad awareness and understanding of how the Sun creates conditions that influence Earth and space, which is increasingly part of the human domain.


Illustration of one of the four identical PUNCH satellites in operation. (Graphic: NASA)

By providing scientists with new information about how these potentially disruptive solar events form and evolve, data from PUNCH could lead to more accurate prediction about the arrival and impact of such events on Earth and for humanity’s robotic explorers in space.

Following orbital adjustments and commissioning, each of these two missions is planned to last for at least two years, contributing valuable data to the study of the universe and the sun’s influence on space weather.

[ANS thanks NASA for the above information]


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ISS Changes Crew for Expedition 73

The 73rd long-duration expedition to the International Space Station (ISS) will begin with the departure of Soyuz MS-26, expected to take place in April 2025. The Expedition 73 crew will consist of astronauts cosmonauts just launched to the station aboard the SpaceX Crew Dragon Endurance, as well as those soon to follow aboard the Soyuz MS-27.

The crew of MS-26, Russian cosmonaunts Alexey Ovchinin and Ivan Vagner and American astronaut Don Pettit, KD5MDT, are already making preparations for departure in the coming weeks.

Scheduled for departure even sooner — probably in the coming week — is SpaceX Crew Dragon Freedom with two members of SpaceX Crew 9, astronaut Nick Hague, KG5TMV, and cosmonaut Aleksandr Gorbunov, accompanied by U.S. astronauts Barry “Butch” Wilmore, and Sunita Williams, KD5PLB. Wilmore and Williams were launched to the ISS in June of last year aboard the Boeing Starliner Crew Flight Test.

The astronauts of NASA’s SpaceX Crew 10 (from left) Kirill Peskov, Nichole Ayers, Takuya Onishi and Anne McClain, leave crew quarters at Kennedy Space Center, FL Wednesday, March 12, 2025 headed for the launch pad. They finally launched to the International Space Station on March 14.
(Photo: Craig Bailey/FLORIDA TODAY via USA TODAY NETWORK)

SpaceX Crew 10 consists of NASA astronaut Anne McClain, who will serve as Crew-10’s commander. She is joined by Crew-10’s pilot, NASA astronaut Nichole Ayers, KJ5GWI, mission specialist Japanese Aerospace Exploration Agency (JAXA) astronaut Takuya Onishi, KF5LKS, and Roscosmos cosmonaut Kirill Peskov. Crew 10 was launched from pad 39A at the Kennedy Space Center in Florida on Friday, March 14, at 23:03 UTC after a scrub on Wednesday. The March 12 launch attempt was scrubbed due to an issue with the hydraulics on ground support systems on the launch pad.

That crew will be joined later next month by the crew of Soyuz MS-27, which is scheduled to consist of cosmonaunts Sergey Ryzhikov and Alexey Zubritsky, as well as American astronaut Jonny Kim.

Once the MS-26 crew departs, Takuya Onishi of the Japan will serve as the commander of Expedition 73, the third JAXA astronaut to take command of the station. Born in Nerima, Japan, Onishi earned an aeronautical and space engineering degree from the University of Tokyo and was a co-pilot of Boeing 767 airplanes from 2003 to 2009. Onishi will fly to space for the second time on Crew-10, having previously flown to the ISS aboard Soyuz MS-01 in 2016 as part of Expedition 48/49. JAXA and NASA selected Onishi for NASA’s 20th astronaut group in 2009.

Expedition 73 will continue the extensive scientific research conducted aboard the ISS, focusing on various fields, including biology, human physiology, physics, and materials science. The crew members will also maintain and upgrade the space station systems.

[ANS thanks NASA for the above information]


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Changes to AMSAT-NA TLE Distribution for 14 March

Two Line Elements or TLEs, often referred to as Keplerian elements or keps in the amateur community, are the inputs to the SGP4 standard mathematical model of spacecraft orbits used by most amateur tracking programs. Weekly updates are completely adequate for most amateur satellites. TLE bulletin files are updated daily in the first hour of the UTC day. New bulletin files will be posted immediately after reliable elements become available for new amateur satellites. More information may be found at https://www.amsat.org/keplerian-elements-resources/.

NOTICE: In an effort to minimize confusion between sources of two line element sets, AMSAT is adopting the convention of listing the USSF/NORAD Satellite Catalog name first, followed by any secondary name or names in parentheses. For example, “POEM 4 (BGS ARPIT)” was added recently where “POEM 4” is the name that appears in the U.S. Space Force Satellite Catalog, and “BGS ARPIT” is the name best known within the amateur satellite community. Expect name changes for affected satellites in the coming weeks as this change is fully implemented.

The following satellite has been added to this week’s AMSAT TLE distribution:
+ HYDRA-T NORAD Cat ID 62692 Downlink 437.778 MHz

[ANS thanks Joe Fitzgerald, KM1P, AMSAT Orbital Elements Manager for the above information]


ARISS NEWS

Amateurs and others around the world may listen in on contacts between amateurs operating in schools and allowing students to interact with astronauts and cosmonauts aboard the International Space Station. The downlink frequency on which to listen is 145.800 MHz worldwide.

None scheduled in the immediate future due to crew changes.

The crossband repeater continues to be active (145.990 MHz up {PL 67} & 437.800 MHz down). If any crewmember is so inclined, all they have to do is pick up the microphone, raise the volume up, and talk on the crossband repeater. So give a listen, you just never know.

The packet system is also active (145.825 MHz up & down).

As always, if there is an EVA, a docking, or an undocking; the ARISS radios are turned off as part of the safety protocol. Systems will be OFF for Crew Dragon docking on March 16, and for undocking later in the week.

Note, all times are approximate. It is recommended that you do your own orbital prediction or start listening about 10 minutes before the listed time.

The latest information on the operation mode can be found at https://www.ariss.org/current-status-of-iss-stations.html

The latest list of frequencies in use can be found at https://www.ariss.org/contact-the-iss.html

[ANS thanks Charlie Sufana, AJ9N, one of the ARISS operation team mentors for the above information]


Upcoming Satellite Operations

+ N4AKV/R will be on various satellites from FM25, FM26, FM27, and FM28 on March 16-18. See hams.at for details.

+ PA3GAN will be on AO-07 from JO22 on March 16.

+ WD5GRW will be on FM satellites for a POTA operation in EM01 on March 16.

A growing number of satellite rovers are currently engaged in sharing their grid square activations on https://hams.at. By visiting the website, you gain easy access to comprehensive information about the operators responsible for activating specific grid squares. Additionally, you have the ability to assess the match score between yourself and a particular rover for a given pass, while also being able to identify the upcoming satellite passes that are accessible from your location.

[ANS thanks hams.at for the above information]


AMSAT Ambassador Activities

AMSAT Ambassadors provide presentations, demonstrate communicating through amateur satellites, and host information tables at club meetings, hamfests, conventions, maker faires, and other events.

March 22, 2025
Midwinter Madness Hamfest
Buffalo Civic Center
1306 County Rd 134
Buffalo MN 55313
https://k0ltc.org/midwinter-madness/
KØJM, ADØHJ, KEØPBR

March 27, 2025
AMSAT Update and Info
West Fork Amateur Radio Club
Paradise Fire Dept.
303 Main St.
Paradise, TX 76073
https://wfarc.org/
W5ITR

April 4 – 5, 2025
Southeastern VHF Conference 2025
Quality Inn
3095 Wilma Rudolph Blvd
Clarksville, TN 37040
https://svhfs.org/wp/2025-conference/
W4FCL

April 5, 2025
RARSfest
Jim Graham Building
NC State Fairgrounds
Youth Center Drive, Gate 5
Raleigh NC
https://www.rarsfest.org/index.php
K4EB, N4AEW, W1DCM, KK4HG, N4HF

[ANS thanks Bo Lowrey, W4FCL, Director – AMSAT Ambassador Program, for the above information]


Satellite Shorts From All Over

+ AMSAT Italia is pleased to announce the renewal of its Board of Directors, which were elected on February 26th and assigned to the role on March 3rd. The new Board of Directors, in charge for the period 2025-2027, consists of:

  • De Paolis Francesco IKØWGF – President / Treasurer
  • Ferrario Gianpietro IZ2GOJ – Vice President
  • Andrioli Fabio IZØQPO – Secretary
  • Ariotti Claudio IK1SLD – Board Member
  • Tognolatti Piero IØKPT – Board Member

Andrioli Fabio IZØQPO and Tognolatti Piero IØKPT join the BoD after being former members of the board of auditors. Fabrizio Carrai IU5GEZ and Emanuele D’Andria IØELE leave the BoD, while Emanuele IØELE was already appointed by the assembly of associates as President Emeritus of AMSAT Italia. For more information about AMSAT Italia and its activities, please visit their website https://www.amsat.it. (ANS thanks Francesco De Paolis, IKØWGF, for the above information.)

+ Intuitive Machine’s IM-2 Athena lander touched down near the Moon’s south pole, 250 meters from its target in the Mons Mouton region, inside of a crater. But, while a softer landing than last time, like IM-1 in Feb 2024, the lander appears to have fallen over into an “incorrect attitude” ending up “somewhat on its side.” A day later the mission was declared over, with little hope of even partial recovery due to solar panels oriented in the wrong direction and the extreme cold temperatures in the crater. (ANS thanks The Orbital Index for the above information.)

+ With somewhat better luck, another private lunar lander carrying a drill, vacuum and other experiments for NASA touched down on the moon on March 2, the latest in a string of companies looking to kickstart business on Earth’s celestial neighbor ahead of astronaut missions. Firefly Aerospace’s Blue Ghost lander descended from lunar orbit on autopilot, aiming for the slopes of an ancient volcanic dome in an impact basin on the moon’s northeastern edge of the near side. (ANS thanks The Associate Press for the above information.)

+ Starship blew up over the Caribbean, again. Starship Flight 8 seems to have suffered the same fate as its predecessor. Eight minutes into Ship 34’s powered flight, four of its six Raptor engines shut down, and the craft began to tumble. Minutes later, it exploded over the Caribbean, producing a similarly spectacular light show as the last flight. In better news, Super Heavy Booster 15 was again caught by its launch tower, an incredible feat that is somehow slowly starting to look routine. (ANS thanks The Orbital Index for the above information.)

+ NASA recently turned off Voyager 1’s cosmic ray subsystem experiment and Voyager 2’s low-energy charged particle instrument to conserve power. At 43 years old, both craft are at half their initial power levels, now operating at around 235W each and losing about 4W of power generation capacity each year. In part, this is due to the 87.7-year half-life decay of Plutonium-238, which powers the probes’ three Multi-Hundred-Watt Radioisotope Thermoelectric Generators. (ANS thanks The Orbital Index for the above information.)


Join AMSAT today at https://launch.amsat.org/

In addition to regular membership, AMSAT offers membership to:

* Societies (a recognized group, clubs or organization).
* Primary and secondary school students are eligible for membership at one-half the standard yearly rate.
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Contact info [at] amsat.org for additional membership information.

73 and remember to help Keep Amateur Radio in Space!

This week’s ANS Editor, Mark Johns, KØJM
mjohns [at] amsat.org

ANS is a service of AMSAT, the Radio Amateur Satellite Corporation, 712 H Street NE, Suite 1653, Washington, DC 20002

ANS-061 AMSAT News Service Bulletins

In this edition:

* Amateur Satellites Scheduled for Launch This Week
* Nine New TEVEL Satellites Scheduled for Launch
* UVSQ-Sat NG Scheduled for Launch
* Intuitive Machines’ Lunar Lander Beams Back First Images of Earth
* SpaceX Delays Flight 8 of Starship
* GridMasterMap Satellite Top 100 Rovers March 2025 Rankings
* VUCC Standings February 2025
* Changes to AMSAT-NA TLE Distribution
* ARISS News
* Upcoming Satellite Operations
* AMSAT Ambassador Activities
* Satellite Shorts From All Over

The AMSAT News Service bulletins are a free, weekly news and information service of AMSAT, the Radio Amateur Satellite Corporation. ANS publishes news related to Amateur Radio in Space including reports on the activities of a worldwide group of Amateur Radio operators who share an active interest in designing, building, launching and communicating through analog and digital Amateur Radio satellites.

The news feed on http://www.amsat.org publishes news of Amateur Radio in Space as soon as our volunteers can post it.

Please send any amateur satellite news or reports to: ans-editor [at] amsat.org

Sign up for free e-mail delivery of the AMSAT News Service Bulletins via the ANS List; to join this list see: https://mailman.amsat.org/postorius/lists/ans.amsat.org/

Amateur Satellites Scheduled for Launch This Week

A SpaceX Falcon 9 rocket will launch a dozens of satellites on the company’s 13th smallsat rideshare mission to a sun-synchronous orbit. The launch is currently scheduled for Tuesday, March 4.

Among those satellites is HADES-ICM 1.5 PocketQube satellite main mission is to act as a FM voice repeater. It can also repeat FSK derived modes like FT-4 and FT-8.

As there is a small empty space available, it will be used to carry an experiment by Smart IR/Graphene Engineering Innovation Centre, GEIC University of Manchester (UK) consisting in a very low power active radiator to be tested on space conditions. The data for this experiment will be transmitted in a specific data packet in the telemetry. This experiment is the same as the one in HADES-R [now SO-124 — see ANS-054]. This experiment will be delivered to AMSAT EA for integration and will be operated by AMSAT-EA, being all its data public and open.

Engineering and manufacturing support for this mission is carried out with the help of private sector companies and universities, but AMSAT-EA will be the only operating organization.

icMercury is a company also supporting the mission. It will develop ground tracking software for the satellite. Telemetry will send some FSK English formatted text messages, part of a history, to be collected as a challenge.

HADES-ICM will offer licensed radio-amateur around the world the opportunity to relay FM voice and AX.25 / APRS 300 / 1200 bps communications. FSK derived transmissions and modes like FT-4 and FT-8 are also supported. As an improvement from previous missions, maximum power is now 0.25W when battery is charged (the amplifier uses battery energy), allowing easier QSOs with handheld antennas like Arrow or Elk and less sensitive receivers.

The satellite will also transmit telemetry with its status and CW messages. This all will be achieved by implementing a SDR based repeater. The FM / FSK repeater will be available all time and opened by squelch level without the need of a subtone.

As payload, the satellite will carry an experiment by Smart IR/Graphene Engineering Innovation Centre, GEIC University of Manchester (UK) consisting in a very low power active radiator to be tested on space conditions. This experiment is the same as the one in HADES-R satellite with updates and improvements. Also, as a challenge made with icMercury, telemetry will send FSK English formatted text messages, part of a history, to be collected.

This satellite is based on the hardware of HADES-D (SO-121, currently being used by hams worldwide for voice contacts) and the next to launch HADES-R. FM satellites are very demanded and appreciated by the ham community because they are easy to use, they don’t require of expensive transceivers and allow continental and even transatlantic contacts in some conditions.

With this satellite we also put into use the amateur VHF and UHF satellite sub-bands helping to secure them for the community in the future. Proposing a UHF downlink and planning a launch on SpaceX Transporter 13 into a 500-600 km polar orbit in Feb 2025. A downlink on 436.666 MHz has been coordinated by the International Amateur Radio Union (IARU).

[ANS thanks IARU for the above information]


The 2025 AMSAT President’s Club Coins Have Just Arrived!
Celebrating the 40th Anniversary of Amateur Radio on Human Spaceflight
Help Support GOLF and Fox Plus.

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Join the AMSAT President’s Club today and help
Keep Amateur Radio in Space!
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Nine New TEVEL Satellites Scheduled for Launch

A group of satellites labeled as “TEVEL2” are on the launch manifest for the SpaceX ransporter 13 mission scheduled for launch on March 4. Designated as TEVEL2-1 through TEVE2-9, they are all listed as having a downlink frequency of 436.400 MHz. However, this frequency has not been coordinated with the International Amateur Radio Union (IARU).

One may assume that these satellites will operate in much the same manner as the first series of TEVEL satellites, launched in January of 2022 and now decayed from orbit. These satellites were activated individually and carried FM repeaters with the same 436.400 MHz downlink, and an uplink frequency of 145.970 MHz. However, there is no official word from the satellite sponsors as to their plans for this new series of satellites.

Yet another satellite on the Transporter 13 manifest is NILA, a 3U cubesat built by HEX20Labs and students of Marian Engineering College, both in India. The builders of this satellite requested a UHF downlink for 9600 bps GFSK/AX25 telemetry. However, the IARU declined the request because they deemed the project commercial, and not qualifying for use of amateur frequencies.

[ANS thanks Jan van Gils, PEØSAT, for the above information]


UVSQ-Sat NG Scheduled for Launch

Also among the satellites on the manifest for the SpaceX Rideshare 13 launch is the third of a series of French cubesats, named UVSQ-Sat NG — or “Next Generation.” The previous satellites in this series carried amateur radio FM transponders.

Specifically designed to observe essential climate variables, UVSQ-Sat NG is a 6U nanosatellite, meaning that it has the dimensions of six stacked unit cubes, each cube having a standard size of 10 centimetres by. Weighing only 10 kg, UVSQ-Sat NG represents a true concentrate of technology. The satellite is equipped with a sophisticated attitude determination and control system designed to meet a variety of scientific requirements related to the observation of essential climate variables. This addition distinguishes it considerably from its two predecessors, UVSQ-Sat and INSPIRE-Sat 7. In a study published in the journal Remote Sensing Journal, a team of researchers from the Atmospheres Laboratory, Space Observations (LATMOS – CNRS/Sorbonne University / UVSQ), in partnership with industry, described this new space mission as well as its scientific aims. The satellite is scheduled to be launched in 2025.

One of the objectives of UPSQ-Sat NG is to maintain the continuity of the Earth’s Radial Assessment studies initiated by the UVSQ-Sat and INSPIRE-Sat 7 satellites, launched in 2021 and 2023 respectively. The UVSQ-Sat NG mission also involves monitoring concentrations of greenhouse gases, such as carbon dioxide and methane, while analysing their links with infrared radiation emitted by the Earth.

In addition to the methods used to determine the components of the Earth’s Radial Balance sheet from the instruments of the UVSQ-Sat NG satellite, researchers detail the technologies used to extract information on atmospheric gas columns (CO2, CH4, O2, H2O) from data from the miniaturised infrared spectrometer that will be on board UPSQ-Sat NG.

Both scientific and innovative, this research project is primarily an educational tool, and is an exceptional educational platform for students who are actively involved in the design, implementation of the satellite structure, and the establishment of a satellite management and management centre. This programme aims to meet the requirements of enterprises and public bodies in terms of training, development of initial and continuous educational programmes, while at the same time increasing the attractiveness of these training courses. This is in order to ensure the acquisition of the key competences required for the emerging professions of France in 2030.

UVSQ-Sat NG is equipped with several instruments, including radiative sensors (thermopiles with carbon nanotubes) for monitoring incoming solar radiation and outgoing terrestrial radiation. A near-infrared spectrometer is also on board to evaluate atmospheric concentrations of greenhouse gases by making observations in the wavelength range of 1200 to 2000 nm.

In addition, UVSQ-Sat NG carries a high-definition camera designed to take images of the Earth in the visible spectrum. This NanoCam will facilitate the post-processing of spectrometer-based data by ensuring accurate geolocation of observed scenes. It will also offer the possibility of observing the Earth’s edge, thus giving an approximate estimation of the vertical temperature profile of the atmosphere.

A scientific paper published in the journal, Remote Sensing states that, “The Isispace VHF Receiver (RX) operates in the commercial frequency range of 148 to 150.5 MHz, and for amateur frequency coordination, it operates within the frequency range of 145.8 to 146.0 MHz. On the other hand, the Isispace VHF Transmitter (TX) covers the commercial frequency range of 400.15 to 402.0 MHz and, for amateur usage, it spans the range of 435.0 to 438.0 MHz. An audio transponder will also be used with the amateur radio community.”

However, no amateur frequencies have been coordinated with the International Amateur Radio Union (IARU) and no amateur operation has been announced.

[ANS thanks Remote Sensing and IARU for the above information]



Intuitive Machines’ Lunar Lander Beams Back First Images of Earth

The Athena lunar lander manufactured by Houston, Texas aerospace company Intuitive Machines shared its first “selfies” from orbit after launching at 00:16 UTC on Thursday, Feb. 27 from the Kennedy Space Center in Florida.

The images released later Thursday show the six-legged Nova-C lander with Earth in the background. Intuitive Machines shared the photos within about 13 hours of the spacecraft launching to orbit aboard a SpaceX Falcon 9 rocket.


Intuitive Machines, the company that built and operates that lunar lander, shared the first images from orbit after launching from Florida. The craft is carrying a number of science instruments, including water-hunting technology for NASA. [Photo: © Intuitive Machines]

The Athena spacecraft, which is on a mission known as IM-2, is now one of two American-made uncrewed lunar landers on their way to the moon’s surface. Firefly Aerospace, also based in Texas, is operating its own spacecraft named Blue Ghost that is due to attempt a landing early Sunday after about a 45-day voyage.

NASA is the primary customer on both commercial spaceflights, which are due to study different regions of the moon’s surface to pave the way for astronauts to return as early as 2027 under the space agency’s Artemis program. The NASA campaign is treating the moon as a vital pit stop for spacefarers to pause and fuel up ahead of the first crewed missions to Mars.

If all goes to plan, Athena should be landing on the moon’s south pole on Thursday, March 6.

The IM-2 mission is targeting a landing near a plateau known as Mons Mouton, which would be even further south than Intuitive Machines’ first lander, Odysseus, which made history in February 2024. The mesa-like lunar mountain towers over a landscape carved by craters, including the Shackleton Crater – a cold, dark region where water ice and other volatile materials that turn easily into gas are thought to be abundant.

The main experiment onboard Athena is NASA’s PRIME-1 (Polar Resources Ice Mining Experiment-1). The dual instrument composed of both a drill and a mass spectrometer will excavate and measure lunar soil, known as regolith, to detect whether gases and accessible resources are present.

Water ice thought to be abundant in the region, once uncovered, could be extracted and used for drinking, breathing and as a source of hydrogen and oxygen for rocket fuel to make future expeditions to Mars possible, according to NASA.

Other objectives include testing a Nokia LTE 4G communications system and deploying a propulsive drone capable of hopping across the lunar surface.

NASA’s Lunar Trailblazer spacecraft, which launched as a rideshare on the Falcon 9, also began its own separate journey to lunar orbit to map the distribution of the different forms of water on Earth’s only natural satellite.

[ANS thanks Eric Lagatta reporting for USA Today for the above information]


SpaceX Delays Flight 8 of Starship

SpaceX has pushed the eighth test flight of its Starship megarocket back a few days.

Elon Musk’s company had been targeting Friday (Feb. 28) for Flight 8 of Starship, the biggest and most powerful rocket ever built. But that’s no longer the plan.

“Now targeting to launch Starship’s eighth flight test as soon as Monday, March 3,” SpaceX said in an X post early on Thursday morning (Feb. 27). No reason was given for the delay.

If all goes to plan, Starship will lift off from Starbase, SpaceX’s facility in South Texas, on Monday during a window that opens at 2330 UTC (5:30 p.m. local Texas time).

SpaceX will try for another “chopsticks” catch of Super Heavy, the booster — its third overall, if successful — and Ship, the upper stage, will attempt to deploy mock Starlink satellites on its suborbital trajectory.

Ship will again target a controlled splashdown off Western Australia. Eventually, SpaceX plans to snag the returning upper stage using the launch tower’s chopsticks as well, but the company isn’t ready to try that just yet.

[ANS thanks Space.com for the above information]


GridMasterMap Satellite Top 100 Rovers March 2025 Rankings

The March 2025 rankings for the Top 100 Rovers (Mixed LEO/MEO/GEO) in satellite operations, as determined by @GridMasterMap on Twitter, has been released. The ranking is determined by the number of grids and DXCC entities activated, taking into account only those grids where a minimum number of QSOs logged on the gridmaster.fr website have been validated by a third party. Grid numbers do not directly reflect the exact number of activations. Satellite operators are encouraged to upload their LoTW satellite contacts to https://gridmaster.fr in order to provide more accurate data.

Updated: 2025-02-28

1 ND9M 26 KX9X 51 W7WGC 76 HB9GWJ
2 NJ7H 27 ON4AUC 52 N6DNM 77 PT2AP
3 JA9KRO 28 KG5CCI 53 JK2XXK 78 AA8CH
4 UT1FG 29 N5BO 54 EA4NF 79 PT9BM
5 N5UC 30 K8BL 55 SM3NRY 80 VE1VOX
6 DL6AP 31 KE4AL 56 JL3RNZ 81 FG8OJ
7 OE3SEU 32 KB5FHK 57 DF2ET 82 YU0W
8 WI7P 33 VE3HLS 58 XE1ET 83 KJ7NDY
9 DP0POL 34 PA3GAN 59 LU4JVE 84 KI7UXT
10 K5ZM 35 KI0KB 60 AA5PK 85 N6UTC
11 F5VMJ 36 JO2ASQ 61 KI7QEK 86 KB2YSI
12 N6UA 37 KI7UNJ 62 SP5XSD 87 AF5CC
13 HA3FOK 38 LA9XGA 63 F4DXV 88 WA9JBQ
14 WY7AA 39 F4BKV 64 AD7DB 89 N4DCW
15 N9IP 40 BA1PK 65 VE1CWJ 90 JM1CAX
16 W5PFG 41 VA3VGR 66 KE9AJ 91 K0FFY
17 LU5ILA 42 N7AGF 67 DL4EA 92 VE3GOP
18 DL2GRC 43 VK5DG 68 N8RO 93 N0TEL
19 AK8CW 44 XE3DX 69 KM4LAO 94 KG4AKV
20 AD0DX 45 KE0WPA 70 VA7LM 95 W8MTB
21 N4AKV 46 PR8KW 71 BG7QIW 96 CU2ZG
22 AD0HJ 47 KE0PBR 72 M1DDD 97 VE7PTN
23 WD9EWK 48 K7TAB 73 W8LR 98 DK9JC
24 ND0C 49 EB1AO 74 W1AW 99 K6VHF
25 DJ8MS 50 AC0RA 75 N4UFO 100 VE6WK

[ANS thanks @GridMasterMap for the above information]


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VUCC Standings February 2025

Here are the firsts from the new VUCC holders for Feb 2025:

N5YIZ is first VUCC Satellite holder from EL08
KH6WI/W9 (EN54) is first VUCC Satellite holder from EN54
W4BB is first VUCC Satellite holder from FM04
G4BWP is first VUCC Satellite holder from JO02
SV8CKM is first VUCC Satellite holder from KM08
SV2DSJ is first VUCC Satellite holder from KN10
ER1KW is first VUCC Satellite holder from Moldova and KN46
RA3LAS is first VUCC Satellite holder from KO85
BG6HXD is first VUCC Satellite holder from OM83
BI8FFH is first VUCC Satellite holder from PM06

[ANS thanks Jon Goering, N7AZ, for the above information.]


Changes to AMSAT-NA TLE Distribution for February 28

Two Line Elements or TLEs, often referred to as Keplerian elements or keps in the amateur community, are the inputs to the SGP4 standard mathematical model of spacecraft orbits used by most amateur tracking programs. Weekly updates are completely adequate for most amateur satellites. TLE bulletin files are updated daily in the first hour of the UTC day. New bulletin files will be posted immediately after reliable elements become available for new amateur satellites. More information may be found at https://www.amsat.org/keplerian-elements-resources/.

The following satellite has been added to this week’s AMSAT TLE distribution:

HADES-R (SO-124) NORAD Cat ID 62690

The following satellites have been deleted from this weeks AMSAT TLE distribution:

SO-120 NORAD Cat ID 56992 Decayed from orbit on or about 11 February 2025
XW-2C NORAD Cat ID 40906 Decayed from orbit on or about 16 February 2026

[ANS thanks Joe Fitzgerald, KM1P, AMSAT Orbital Elements Manager for the above information]


ARISS NEWS

Amateurs and others around the world may listen in on contacts between amateurs operating in schools and allowing students to interact with astronauts and cosmonauts aboard the International Space Station. The downlink frequency on which to listen is 145.800 MHz worldwide.

FAILED
Royal Moroccan Air Academy, Marrakech, Morocco, direct via CN8ERA
The ISS callsign was scheduled to be OR4ISSThe scheduled crewmember was Sunita Williams, KD5PLB
The ARISS mentor is IN3GHZ
Contact was not successful for: Fri 2025-02-21 11:12:20 UTC 72 degrees maximum elevation
ARISS is working to determine what exactly happened.

UPCOMING
No additional contacts are scheduled in the immediate future.

The crossband repeater continues to be active (145.990 MHz up {PL 67} & 437.800 MHz down). If any crewmember is so inclined, all they have to do is pick up the microphone, raise the volume up, and talk on the crossband repeater. So give a listen, you just never know.

The packet system is also active (145.825 MHz up & down).

As always, if there is an EVA, a docking, or an undocking; the ARISS radios are turned off as part of the safety protocol.

Note, all times are approximate. It is recommended that you do your own orbital prediction or start listening about 10 minutes before the listed time.

The latest information on the operation mode can be found at https://www.ariss.org/current-status-of-iss-stations.html

The latest list of frequencies in use can be found at https://www.ariss.org/contact-the-iss.html

[ANS thanks Charlie Sufana, AJ9N, one of the ARISS operation team mentors for the above information]


Upcoming Satellite Operations

Kyle Chavis, WA4PGM, will be QRV from St. Lucia from 26 Feb through 4 Mar as J68HZ. OPERATION SUSPENDED DUE TO EXTREME WEATHER. Keep an eye on hams.at for additional info.

Tom Gaines, KB5FHK, plans operations from EM62 and from EM72 on March 8 & 9. See hams.at for details.

A growing number of satellite rovers are currently engaged in sharing their grid square activations on https://hams.at. By visiting the website, you gain easy access to comprehensive information about the operators responsible for activating specific grid squares. Additionally, you have the ability to assess the match score between yourself and a particular rover for a given pass, while also being able to identify the upcoming satellite passes that are accessible from your location.

[ANS thanks Ian Parsons, K5ZM, AMSAT rover page manager, for the above information]


AMSAT Ambassador Activities

AMSAT Ambassadors provide presentations, demonstrate communicating through amateur satellites, and host information tables at club meetings, hamfests, conventions, maker faires, and other events.

March 1, 2025
Irving Hamfest
Betcha Bingo Hall
2420 W. Irving Blvd.
Irving, TX 75014
http://irvingarc.org/hamfest
N5HYP

March 22, 2025
Midwinter Madness Hamfest
Buffalo Civic Center
1306 County Rd 134
Buffalo MN 55313
https://k0ltc.org/midwinter-madness/
KØJM, ADØHJ, KEØPBR

April 4 – 5, 2025
Southeastern VHF Conference 2025
Quality Inn
3095 Wilma Rudolph Blvd
Clarksville, TN 37040
W4FCL

April 5, 2025
RARSfest
Jim Graham Building
NC State Fairgrounds
Youth Center Drive, Gate 5
Raleigh NC
https://www.rarsfest.org/index.php
K4EB, N4AEW, W1DCM, KK4HG, N4HF

[ANS thanks Bo Lowrey, W4FCL, Director – AMSAT Ambassador Program, for the above information]


Satellite Shorts From All Over

+ A total lunar eclipse will happen overnight between March 13 and March 14, 2025. It will be the first total lunar eclipse visible anywhere in the world since November 2022, and will also be the first of three happening between 2025 and 2026. During totality — the peak phase of the eclipse — the moon will turn a deep reddish-orange hue, earning it the nickname “Blood Moon.” This effect happens because Earth’s atmosphere scatters shorter wavelengths of light from the sun while allowing longer wavelengths of red and orange hues to be refracted into Earth’s umbra (the darkest part of Earth’s shadow). When these longer wavelengths strike the moon, they can make it appear red, similar to how the sky appears red during sunrise and sunset. Totality will last for an impressive 65 minutes, beginning at 0726 UTC on March 14. (ANS thanks Space.com for the above information.)

+ GOES-19 will replace GOES-16 as the operational GOES-East weather satellite on April 4, 2025. Between 17 March 2025 and 1 April 2025, the GOES-16 satellite will undergo a minor East/West station-keeping maneuver, drifting from its current operational longitude of 75.2°W to a new operational longitude of 75.5°W. During this time, the GOES-East HRIT/EMWIN Broadcast will continue from GOES-16. This 0.3°W shift is expected to induce minimal change in received signal strength for ground stations employing properly aligned small aperture antennas. GOES-19 will also begin its drift maneuver– drifting from 89.5°W to 75.2°W ~1 deg/day drift. On April 1, GOES 19 arrives at 75.2°W, then GOES-19 Post-Drift Product Checkout at new location commences. (ANS thanks Carl Reinemann, usradioguy.com, for the above information.)

+ In less than 48 hours the HB9RG Trophy of the AMSAT-HB will start. Further information has been added to the website, including the form for entering QSO data as well as provisional activity planning for the bonus day on March 10th: https://www.amsat-hb.org/hb9rg_trophy/hb9rg_trophy_2025_-_distance   QSO with station HB9RG will be rewarded with an additional 500 points on March 10th. Anyone who only wants to contact the HB9RG station on March 10 is invited to do so. Every QSO on March 10 will be confirmed with an anniversary QSL card. Share your activities for the HB9RG Trophy with us via X, Bluesky and Facebook. Use the hashtag #HB9RGTrophy. (ANS thanks Michael Lipp, HB9WDF, President AMSAT-HB, for the above information.)


Join AMSAT today at https://launch.amsat.org/

In addition to regular membership, AMSAT offers membership to:

* Societies (a recognized group, clubs or organization).
* Primary and secondary school students are eligible for membership at one-half the standard yearly rate.
* Post-secondary school students enrolled in at least half time status shall be eligible for the student rate for a maximum of 6 post-secondary years in this status.
* Memberships are available for annual and lifetime terms.

Contact info [at] amsat.org for additional membership information.

73 and remember to help Keep Amateur Radio in Space!

This week’s ANS Editor, Mark Johns, KØJM
mjohns [at] amsat.org

ANS is a service of AMSAT, the Radio Amateur Satellite Corporation, 712 H Street NE, Suite 1653, Washington, DC 20002

ANS-357 AMSAT News Service Weekly Bulletins

In this edition:

* Taiwan’s PARUS-T1A Launch Failed
* NASA Astronauts Face More Time In Space With Return Delayed
* NASA Now Knows Why Its Mars Helicopter Crashed
* Changes to AMSAT-NA TLE Distribution
* ARISS SSTV Event December 25 – January 5
* ARISS News
* Upcoming Satellite Operations
* AMSAT Ambassador Activities
* Satellite Shorts From All Over

The AMSAT News Service bulletins are a free, weekly news and information service of AMSAT, the Radio Amateur Satellite Corporation. ANS publishes news related to Amateur Radio in Space including reports on the activities of a worldwide group of Amateur Radio operators who share an active interest in designing, building, launching and communicating through analog and digital Amateur Radio satellites.

The news feed on http://www.amsat.org publishes news of Amateur Radio in Space as soon as our volunteers can post it.

Please send any amateur satellite news or reports to: ans-editor [at] amsat.org

You can sign up for free e-mail delivery of the AMSAT News Service Bulletins via the ANS List; to join this list see: https://mailman.amsat.org/postorius/lists/ans.amsat.org/

ANS-357 AMSAT News Service Weekly Bulletins

To: All RADIO AMATEURS
From: Radio Amateur Satellite Corporation
712 H Street NE, Suite 1653
Washington, DC 20002

DATE 2024 Dec. 22

Taiwan’s PARUS-T1A Launch Failed

Radio Amateurs around the world were anticipating a new FM repeater in space as a Christmas present this year, but it seems they will find only coal in their stockings. The rocket carrying the PARUS T1A satellite failed to reach orbit.

Space One, a Japanese space startup, said its second attempt to launch a rocket carrying satellites into orbit had been aborted minutes after liftoff Wednesday and destroyed itself, nine months after the company’s first launch attempt ended in an explosion.

Space One’s Kairos No. 2 rocket lifted off from a coastal site in the mountainous prefecture of Wakayama in central Japan. The company said it had aborted the flight after concluding that it was unlikely to complete its mission.

“We are very sorry that we could not achieve as far as a final stage of the mission,” Space One President Masakazu Toyoda told a news conference Wednesday. “We don’t consider this a failure because we are getting valuable data that will help our pursuit toward a next challenge.”

He said he hoped to find the cause to address the problems as soon as possible to achieve a success next time.

Company executive and space engineer Mamoru Endo said the abnormality in the first stage engine nozzle or its control system is likely to have caused an unstable flight of the rocket, which started spiraling in midflight and eventually destroyed itself about three minutes after liftoff, using its autonomous safety mechanism.

The Kairos No. 2 rocket was carrying five small satellites, including one from the Taiwanese space agency and several from Japanese startups. The Taiwanese satellite was PARUS-T1A a 3U CubeSat that featured an FM crossband repeater, as well as an APRS digipeater to provide global amateur activities at the same frequency of ISS APRS channel 145.825MHz.

A second Taiwanese amateur satellite, PARUS-T1, carrying an APRS store-and-forward system, is still scheduled for launch next month on a SpaceX mission. Both satellites were constructed by students at National Formosa University.

Space One said it had fixed the cause of the debut flight failure, which stemmed from a miscalculation of the rocket’s first-stage propulsion.

Japan hopes the company can pave the way for a domestic space industry that competes with the United States.

[ANS thanks the Associated Press and reporter Mari Yamaguchi for the above information]


The 2024 AMSAT President’s Club coins are still available!

Only 10 Days Left!!!

Help Support GOLF and Fox Plus

Join the AMSAT President’s Club today and help
Keep Amateur Radio in Space!
https://www.amsat.org/join-the-amsat-presidents-club/


NASA Astronauts Face More Time In Space With Return Delayed

NASA announced on Tuesday the latest delay in the homecoming for Butch Wilmore and Suni Williams, KD5PLB. Their space mission was extended again. That means they won’t be back on Earth until spring, 10 months after rocketing into orbit on Boeing’s Starliner capsule.

The two test pilots planned on being away just a week or so when they blasted off June 5 on Boeing’s first astronaut flight to the International Space Station. Their mission grew from eight days to eight months after NASA decided to send the company’s problem-plagued Starliner capsule back empty in September.

Now the pair won’t return until the end of March or even April because of a delay in launching their replacements, according to NASA.

NASA shared a holiday snapshot of astronauts Don Pettit and Suni Williams on Dec. 17. [Credit: NASA Johnson]

NASA’s next crew of four was supposed to launch in February, followed by Wilmore’s and Williams’ return home by the end of that month alongside two other astronauts. But SpaceX needs more time to prepare the brand new capsule for liftoff. That launch is now scheduled for no earlier than late March.

Last month, news articles suggesting that Ms. Williams was experiencing health problems during her unplanned extended stay in orbit set off widespread rumors on social media. NASA’s medical chief, Dr. James Polk, assured the public on November 14 that Williams is healthy and not suffering from any medical problems.

“I think there’s some rumors around outside there that I’m losing weight and stuff,” Williams said in an interview on November 12. “No, I’m actually right at the same amount. Things shift around quite a bit, you know? ”

Not only is she healthy, according to her and NASA, but they made Williams commander of Expedition 72 crew. As KD5PLB, she continues to be an active participant in ARISS contacts during her time aboard the ISS.

[ANS thanks The Washington Post, Space.com, and NASA for the above information]


Need new satellite antennas?
Purchase M2 LEO-Packs from the AMSAT Store.

When you purchase through AMSAT, a portion of the proceeds goes towards
Keeping Amateur Radio in Space.
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NASA Now Knows Why Its Mars Helicopter Crashed

Investigating an aircraft crash is no simple task here on Earth. Imagine how much more difficult it would be to diagnose a helicopter accident that took place 69 million miles away with none of the usual data present to help. NASA had to do just that after its Ingenuity Mars Helicopter suffered an accident on Jan. 18, 2024, that has since left it grounded in a crater on Mars. And now, after months of collecting data, the space agency may have finally figured out what happened.

On April 19, 2021, the NASA Ingenuity Mars Helicopter made history by lifting off the Jezero Crater’s floor and becoming the first aircraft to fly on a celestial entity other than Earth. The helicopter was supposed to fly only five experimental flights over 30 days to demonstrate that flight on Mars was possible. But it exceeded all expectations, conducting 72 flights over three years, setting all sorts of altitude records in the process, ending with that early 2024 accident.

The wreckage of the Inguity Mars Helicopter as seen by the Mars Rover Perseverance. The helicopter is on the right and the broken rotor is approximately 49 feet away on the left. [Photo: NASA/JPL-Caltech/LANL/CNES/CNRS]

The final moments of the helicopter’s flight were more or less a mystery at first. Ingenuity lifted off like it had 71 times before. Then camera footage showed that it began initiating descent after just 19 seconds of flight. By the time 32 seconds had elapsed, the helicopter was on the Martian surface again and had halted communications. Six days later, the helicopter beamed back images that showed it had sustained severe rotor-blade damage and would no longer be able to fly.

Now, NASA believes that the navigation system was ultimately to blame. The navigation system used the helicopter’s downward-facing camera to track visual features on the ground. During this final flight, the helicopter was flying over a portion of the Jezero Crater that is known for textured, featureless sand ripples. The navigation system was thus unable to find any suitable ground features to track for a landing.

From there, several things went wrong. NASA says that the helicopter made hard contact with a sand-ripple slope, causing it to pitch and roll. The sudden change in altitude was too much for the rotor blades, and four of them broke off at their weakest points. This caused the rotor system to vibrate excessively, which ripped one of the blades clean off. Finally, the incident generated an excessive power draw that caused communications to fail.

NASA’s graphic depicts the most likely scenario for the accident, in which Ingenuity landed hard on a sand-ripple slope, causing irreparable rotor-blade damage.
[NASA/JPL-Caltech]

“When running an accident investigation from 100 million miles away, you don’t have any black boxes or eye witnesses,” said Håvard Grip, Ingenuity’s first pilot and research technologist at JPL Robotics. “While multiple scenarios are viable with the available data, we have one we believe is most likely: Lack of surface texture gave the navigation system too little information to work with.”

Nobody expected Ingenuity to last as long as it did. Its flights gave researchers excellent aerial views of our red neighbor. Even now, as it lies in the sands of the Jezero Crater, Ingenuity can no longer fly but still beams back weather and avionics data to NASA. The avionics data along with the flight data from Ingenuity’s 72 flights — combined with Ingenuity’s incredible longevity — are helping NASA develop smaller, lighter avionics for future aircraft on Mars.

“Because Ingenuity was designed to be affordable while demanding huge amounts of computer power, we became the first mission to fly commercial off-the-shelf cellphone processors in deep space,” said Ingenuity project manager Teddy Tzanetos. “We’re now approaching four years of continuous operations, suggesting that not everything needs to be bigger, heavier and radiation-hardened to work in the harsh Martian environment.”

Tzanetos and his team are already working on another Mars helicopter. It’s approximately 20 times heavier than the Ingenuity and is being designed to carry several pounds of science equipment while autonomously exploring remote locations on Mars.

[ANS thanks CNET.com and space reporter Joe Hindy for the above information]


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Changes to AMSAT-NA TLE Distribution for Dec. 20

Two Line Elements or TLEs, often referred to as Keplerian elements or keps in the amateur community, are the inputs to the SGP4 standard mathematical model of spacecraft orbits used by most amateur tracking programs. Weekly updates are completely adequate for most amateur satellites. TLE bulletin files are updated daily in the first hour of the UTC day. New bulletin files will be posted immediately after reliable elements become available for new amateur satellites. More information may be found at https://www.amsat.org/keplerian-elements-resources/.

This week there are no additions or deletions to the AMSAT TLE distribution.

[ANS thanks Joe Fitzgerald, KM1P, AMSAT Orbital Elements Manager for the above information]


ARISS SSTV Event December 25 – January 5

[ANS thanks ARISS for the above information.]


ARISS NEWS

Amateurs and others around the world may listen in on contacts between amateurs operating in schools and allowing students to interact with astronauts and cosmonauts aboard the International Space Station. The downlink frequency on which to listen is 145.800 MHz worldwide.

RECENTLY COMPLETED:
Zespół Szkół Łączności, Warszawa, Poland, direct via SP5KAB
The ISS callsign was presently scheduled to be OR4ISS
The scheduled crewmember was Nick Hague, KG5TMV
The ARISS mentor was SP3QFE
Contact was successful: Mon 2024-12-16 08:35:06 UTC 71 degrees maximum elevation.
Congratulations to the Zespół Szkół Łączności students, Nick, mentor SP3QFE, and ground station SP5KAB!
Watch for Livestream at https://www.youtube.com/live/DBafZYpxolI

Sally Ride Elementary School, Orlando, Florida, direct via K1AA
The ISS callsign was presently scheduled to be NA1SS
The scheduled crewmember was Sunita Williams, KD5PLB
The ARISS mentor was AA4KN
Contact was successful: Tue 2024-12-17 18:49:38 UTC 30 degrees maximum elevation.
Congratulations to the Sally Ride Elementary School students, Sunita, mentor AA4KN, and ground station K1AA!
Watch for Livestream at https://youtube.com/live/DuCNyWOPxH0?feature=share

UPCOMING:
ARISS school contacts are currently planned to resume the week of 2025-01-13 to 2025-01-19.

Many times a school may make a last minute decision to do a Livestream or run into a last minute glitch requiring a change of the URL but we at ARISS may not get the URL in time for publication. You can always check https://live.ariss.org/ to see if a school is Livestreaming.

The crossband repeater continues to be ACTIVE (145.990 MHz up {PL 67} & 437.800 MHz down). If any crewmember is so inclined, all they have to do is pick up the microphone, raise the volume up, and talk on the crossband repeater. So give a listen, you just never know.

The packet system is also active (145.825 MHz up & down) until December 25, when the SSTV event begins.

Ham TV – STATUS – Stowed. ​​ Default mode is for​​​ scheduled digital amateur television operations (2395.00 MHz down)​​.

As always, if there is an EVA, a docking, or an undocking; the ARISS radios are turned off as part of the safety protocol. ​Powering OFF for U.S. EVA on Jan 23. ON TBD.

Note, all times are approximate. It is recommended that you do your own orbital prediction or start listening about 10 minutes before the listed time.

The latest information on the operation mode can be found at https://www.ariss.org/current-status-of-iss-stations.html

The latest list of frequencies in use can be found at https://www.ariss.org/contact-the-iss.html

[ANS thanks Charlie Sufana, AJ9N, one of the ARISS operation team mentors for the above information]


Upcoming Satellite Operations

None announced at this time.

A growing number of satellite rovers are currently engaged in sharing their grid square activations on https://hams.at. By visiting the website, you gain easy access to comprehensive information about the operators responsible for activating specific grid squares. Additionally, you have the ability to assess the match score between yourself and a particular rover for a given pass, while also being able to identify the upcoming satellite passes that are accessible from your location.

[ANS thanks Ian Parsons, K5ZM, AMSAT rover page manager, for the above information]


AMSAT Ambassador Activities

AMSAT Ambassadors provide presentations, demonstrate communicating through amateur satellites, and host information tables at club meetings, hamfests, conventions, maker faires, and other events.

February 14-15, 2025
Yuma HAMCON and Southwestern Division Convention
Yuma County Fairgrounds
Yuma, AZ
https://www.yumahamfest.com/
N1UW

[ANS thanks Bo Lowrey, W4FCL, Director – AMSAT Ambassador Program, for the above information]


Satellite Shorts From All Over

+ AO-73 (a.k.a. FUNcube 1) has been switched from autonomous mode to continuous transponder mode for the holiday period. This means that the transponder is available for use 24/7. AO-73 is anticipated to revert to autonomous mode sometime after January 5, 2025. In autonomous mode, the transponder is only available when the satellite is in eclipse. (ANS thanks AMSAT-UK for the above information.)

+ Two Chinese astronauts aboard their country’s orbiting space station spent nine hours working outside in the cold vacuum of space, the longest recorded spacewalk, the Chinese space administration has said. The astronauts on China’s Shenzhou-19 mission, Cai Xuzhe and Song Lingdong, finished their first “extravehicular activities” — spacewalking in popular parlance — this week, apparently nudging past the previous record of eight hours and 56 minutes set by two American astronauts in 2001, according to China’s Manned Space Agency. The feat was another sign of China’s ambitions to project its power and prestige in space. (ANS thanks The New York Times for the above information.)

+ The internet news site MSN recently published a feature on the history of amateur radio and astronauts in orbit, beginning with Owen Garriott, W5LFL, in 1983 and continuing to the present ARISS program. “How Amateur Radio Is Connecting Astronauts In Space With Kids On Earth” was written by Leonard David. See it at http://bit.ly/4gnfE3y (ANS thanks msn.com for the above information.)

+ The first Block 2 version of the giant SpaceX Starship, Ship 33, recently rolled out for testing and completed its first static fire test. It will be stacked on Booster 14 before it is targeted to complete the first flight of the Block 2 reusable upper stage in January. This upgraded Ship adds catch hardware and an additional ring, making it 1.8 m taller and now totaling 124.4 m (408 feet) when eventually stacked on top of Booster 14. The added height will allow it to pack 300 tons more propellant. (ANS thanks The Orbital Index for the above information.)

+ Your AMSAT News Service volunteer editors, Mark Johns, KØJM; Paul Stoetzer, N8HM; Frank Karnauskas, N1UW; and Mitch Ahrenstorff, ADØHJ, wish all of our readers the happiest of holidays.


Join AMSAT today at https://launch.amsat.org/

In addition to regular membership, AMSAT offers membership to:

* Societies (a recognized group, clubs or organization).
* Primary and secondary school students are eligible for membership at one-half the standard yearly rate.
* Post-secondary school students enrolled in at least half time status shall be eligible for the student rate for a maximum of 6 post-secondary years in this status.
* Memberships are available for annual and lifetime terms.

Contact info [at] amsat.org for additional membership information.

73 and remember to help Keep Amateur Radio in Space!

This week’s ANS Editor, Mark Johns, KØJM
mjohns [at] amsat.org

ANS-329 AMSAT News Service Weekly Bulletins

In this edition:

* The Space Age, Morse Code and STEM Innovation
+ ASRTU-1 Designated ASRTU-OSCAR 123
* CubeSatSim Kits Available Once Again (Revised)
* New Chinese Satellite Completes Frequency Coordination
* Update on PARUS-T1A Satellite
* Air Leak on ISS Russian Module Is Getting Worse
* Changes to AMSAT-NA TLE Distribution
* Space Station Raises Orbit Avoiding Orbital Debris
* ARISS News
* Upcoming Satellite Operations
* AMSAT Ambassador Activities
* Satellite Shorts From All Over

The AMSAT News Service bulletins are a free, weekly news and information service of AMSAT, the Radio Amateur Satellite Corporation. ANS publishes news related to Amateur Radio in Space including reports on the activities of a worldwide group of Amateur Radio operators who share an active interest in designing, building, launching and communicating through analog and digital Amateur Radio satellites.

The news feed on http://www.amsat.org publishes news of Amateur Radio in Space as soon as our volunteers can post it.

Please send any amateur satellite news or reports to: ans-editor [at] amsat.org

You can sign up for free e-mail delivery of the AMSAT News Service Bulletins via the ANS List; to join this list see: https://mailman.amsat.org/postorius/lists/ans.amsat.org/

ANS-329 AMSAT News Service Weekly Bulletins

To: All RADIO AMATEURS
From: Radio Amateur Satellite Corporation
712 H Street NE, Suite 1653
Washington, DC 20002

DATE 2024 Nov 24

AMSAT OSCAR-7 50th Anniversary — The Space Age, Morse Code and STEM Innovation

At first glance, there is something about Morse Code and the space age that don’t go together. But, think about Morse in its simple beauty.

In addition to building a few spacecraft and pursuing a global amateur radio allocation for satellites at the International Telecommunications Union World Radio Conference, AMSAT was also busy developing an educational curriculum. Before STEM (Science, Technology, Engineering and Mathematics) was even a concept, AMSAT thought it would be quite exciting to allow grade-school to high-school students the opportunity to understand the basics of a spacecraft — not by reading about it in a book, rather by using a real spacecraft, in class.

Artist rendering of AO-7

One of AMSAT’s members, Dr. Martin Davidoff, K2UBC, decided to write a curriculum at the secondary education level and received a grant from the Department of Energy to write it. The Satellite Experimenters Handbook was distributed by the American Radio Relay League (ARRL) and AMSAT to anyone who might want to teach others about spacecraft technology. The book especially targeted secondary school educators. Key among the concepts was the idea of giving a teacher, who may or may not be a radio amateur, the information necessary to assemble a receiving system, which could act as a student demonstration tool in school. This receiver and antenna would allow a class to “receive and decode” telemetry. This process, then, required the students to think through some orbital mechanics, the technology of antennas and receivers, and finally, the principles of demodulation and decoding.

This is where Morse came in. For just the numbers, 0-9, in Morse can be learned in 10 minutes by just about anyone. And, so it is a perfect tool for any eighth grader!

The Morse Code Telemetry Encoder System (TLM) was designed and fabricated by John Goode, W5CAY. This unit was built in one of the small modules that comprised the AO-7 spaceframe. This little box used fixed logic comprised of 34 IC’s and one op-amp for the A/D converter. Using CMOS components was amazingly efficient; it required 2 mA of current at 10V DC from the power bus – a whopping 20 mW!

This TLM encoder had 24 analog input channels that were organized in 4 columns and 6 rows. They were divided, basically, into current, voltage and temperature channels. All were scaled to a 1.0 V full- scale input to the A/D converter. The encoder produced decimal values and was organized into two Morse characters between 0 and 99. The first number of each word is a digit giving the row number of the datum. This reduces the ambiguity of where in the frame the encoder was; in case the student got a bit lost.

AMSAT’s commitment to STEM education continues today with its CubeSat Simulator program and its developing Youth Initiative – all fueled by a fifty-year-old satellite that is still in operation today.

Persons wanting to read more about the life and history of AMSAT OSCAR-7 are invited to visit https://www.amsat.org/amsat-ao-7-a-fifty-year-anniversary/.

[ANS thanks Frank Karnauskas, N1UW, AMSAT VP-Development, for the above information]


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ASRTU-1 Designated ASRTU-OSCAR 123

At the request of Harbin Institute of Technology and Amur State University, AMSAT has designated ASRTU-1 as ASRTU-OSCAR 123 (AO-123).


Illustration of AO-123 [Credit: nanosats.eu]

ASRTU-1 was launched on November 4, 2024 at 23:18 UTC, on a Soyuz launch vehicle from Vostochny Cosmodrome, Russia. Built and operated by Harbin Institute of Technology and Amur State University, the satellite carries a V/U repeater, UHF SSDV digital image transmitter, and a 10.5 GHz QPSK image transmitter. All of these payloads have been successfully tested, and the repeater has been operational for QSOs.

The satellite contains an FM transponder, which is currently operational, with an uplink of 145.850 MHz (67 Hz CTCSS tone required) and a downlink of 435.400 MHz. After the repeater detects the end of uplink, it will wait for 0.5s. If no new uplink in 0.5s, telemetry will be sent. So make fast QSOs so the telemetry is less like to interrupt you.

The satellite also contains two cameras with an SSDV downlink for low resolution images on 436.210 MHz, and a high speed downlink on 10.460 GHz for high resolution images.

Windows software for decoding telemetry is available at https://drive.google.com/file/d/1W8nm-P0_h0J1Bd1eif74mLo-EuRdWcjH
Two-Line Keplerian elements (TLEs) may be found at http://asrtu.mqsi.xyz/ASRTU_TLE.txt

AMSAT congratulates the Harbin Institute of Technology and Amur State University, thanks them for their contribution to the amateur satellite community, and wishes them continued success on this and future projects.

ANS thanks Drew Glasbrenner, KO4MA, OSCAR Number Administrator, for the above information.]


CubeSatSim Kits Available Once Again (Revised)

Another batch of CubeSatSim Kits will be available on the AMSAT Store on Monday, November 25 starting at noon U.S. Eastern time (1700 UTC). Due to an error, previous announcements had included an earlier date.

The $400 kits include everything you need to assemble a CubeSat Simulator with no soldering. Only about an hour and half of assembly is required to stack the boards, assemble the frame, and mount the solar panels.

The CubeSatSim Kit includes:

  • Fully assembled and tested PCBs (Main, Solar, and Battery Boards)
  • Raspberry Pi Zero 2 with a Pi Camera and fully programmed micro-SD card, along with a fully programmed Raspberry Pi Pico WH
  • AMSAT logo Remove Before Flight tag switch
  • 3D printed frame, nylon screws, and nuts, with a mini screwdriver included for assembly
  • Metal standoffs, stacking headers, and JST jumpers for stacking the PCBs and Pi Zero 2
  • 10 solar panels with pre-soldered JST connectors and mounting tape
  • BME280 sensor (pressure, temperature, altitude, humidity) and MPU6050 IMU/gyro pre-soldered
  • Two 6″ SMA coax cables and two SMA antennas

The kit also comes with an instruction sheet, parts inventory, and links to online instructions. Assembly time is estimated to be under two hours, with scissors and the provided mini screwdriver.

Limited quantities of the CubeSatSim Kit will soon be available for purchase from the AMSAT Store. [Credit: Alan Johnston, KU2Y]

The v2.0 CubeSatSim features improvements over v1.2, such as an FM transceiver, Raspberry Pi Pico microcontroller, and RF command and control using DTMF or APRS packets. It can also be modified to function as a 500mW high altitude balloon payload.

For those interested in creating their own CubeSatSim, v2.0 blank PCB sets are available at the AMSAT Store for $35. These require additional components, which can be purchased for approximately $300 using the provided Bill of Materials.

Additional resources include:

For more information or to borrow a loaner CubeSat Simulator, contact Alan Johnston, AMSAT VP Educational Relations, at ku2y [at] arrl.net.

How to Order
Kits will be sold exclusively on the AMSAT Store website, https://www.amsat.org/product/cubesatsim-kit/. Only U.S. shipping addresses are eligible; orders with non-U.S. addresses will be refunded and closed.

About CubeSatSim
CubeSatSim is a low-cost satellite emulator powered by solar panels and batteries. It transmits UHF radio telemetry and can be expanded with additional sensors and modules, making it ideal for educational and public demonstrations.

[ANS thanks Alan Johnston, KU2Y, AMSAT Vice President Educational Relations for the above information]


New Chinese Satellite Completes Frequency Coordination

The satellite frequency coordination committee of the International Amateur Radio Union (IARU) on November 15 completed approval of frequency requests from the Chinese Amateur Satellite Group (CAMSAT) for a new amateur satellite to be launched next year.

CAS-11, a 6U CubeSat will include:

  • HF/UHF – H/U Mode Linear Transponder, with a bandwidth of 15kHz downlink centered at 435.505 MHz, EIRP 24 dBm
    Uplink 21.320 MHz +/- 7.5 kHz.
  • VHF/UHF – V/U Mode Linear Transponder, with a bandwidth of 30kHz downlink centered at 435.540 MHz, EIRP 24 dBm.
    Uplink 145.860 MHz +/- 15 kHz.
  • VHF/UHF – V/U Mode FM Transponder, downlink at 435.600 MHz, EIRP 24 dBm
    Uplink at 145.925 MHz
  • VHF/UHF – V/U Mode digital store-and-forward Transponder, downlink at 435.700 MHz, EIRP 24 dBm
    Uplink at 145.895 MHz
  • UHF – CW Telemetry Beacon and
  • UHF telemetry beacon using AX.25 4.8k/9.6kbps GMSK at 435.570 MHz, EIRP 23 dBm.

The above transponders and beacon will work 24/7 when the satellite power supply is sufficient. Amateur radio enthusiasts around the world can use it for two-way radio relay communication, data storage and forwarding communication, and receive satellite CW beacons.

The CAS-11 satellite will also be equipped with a 2.4 GHz multi-mode amateur radio satellite beacon transmitter, which is designed and built by university students, high school students and primary school students from Beijing Donggaodi Science and Technology Museum and Beijing University of Posts and Telecommunications under the guidance of CAMSAT. This is an unprecedented satellite project in China. It has brought opportunities for learning and practicing amateur radio and amateur satellites to students of all grades from elementary school to university, and promoted the application of amateur radio in space. This 2.4 GHz experimental beacon transmitter can switch to transmit five different modes of radio signals, and it will work continuously when the satellite is fully powered.

This project aims to cultivate students’ knowledge, skills and interests in amateur radio satellites. All transmission modes operate at 2.4 GHz, and the working modes are converted by the on-board computer program and ground remote control commands. It can work in the following modes: CW Telemetry Beacon, FT8 Telemetry Beacon, PPM Telemetry Beacon, or USB/SSTV Robot36, PD120 1. This beacon will transmit at 2405.500 MHz, EIRP 27 dBm.

CAS-11 carries three cameras, and the photos it takes are stored in the flash memory on the satellite. The builders have designed a simple remote control system based on DTMF commands. Amateur radio enthusiasts around the world can send DTMF commands to download the photo catalog and all photos taken by all cameras.

Anticipating a launch in September, 2025 into a 536 km polar orbit from Haiyang Sea Launch Platform, Shandong, China.

[ANS thanks IARU and Alan Kung, BA1DU, of CAMSAT for the above information.]


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Update on PARUS-T1A Satellite

The satellite frequency coordination committee of the International Amateur Radio Union (IARU) on November 20 updated information regarding the approved frequency requests from the National Formosa University for satellite PARUS-T1A. The satellite is tentatively scheduled for launch in January.

PARUS-T1A, a 3U CubeSat, is designed to continue the successful legacy of the PARUS- T1 mission. This satellite will provide essential services to the global amateur radio community.

The Primary Mission is an FM Voice Cross-Band Repeater to facilitate real-time voice communication between amateur radio operators on 145.980 MHz (Uplink tone 67Hz) and 435.250 MHz (Downlink).

The satellite will also carry an APRS Digipeater to enable the transmission of real-time position and status information from APRS-equipped devices on 145.825 MHz.

A telemetry beacon downlink on 437.850 MHz has also been coordinated, with unencrypted telemetry packets accessible to the public through online dashboards like SatNOGS, promoting transparency and community collaboration.

Anticipating a SpaceX launch from Florida in January, 2025 into a 590 x 510 km 98 degree orbit.

[ANS thanks IARU and Randson Huang, BV2DQ, for the above information.]


Air Leak on ISS Russian Module Is Getting Worse

For the past five years, air has been escaping through a Russian section of the International Space Station (ISS) at an increasing rate. NASA and its Russian counterpart, Roscosmos, are still in disagreement over the root cause of the leak, as well as the severity of the consequences.

The leak was first discovered in 2019 in the vestibule (named PrK) that connects a docking port to the Russian Zvezda module, which Roscosmos had launched to low Earth orbit in July 2000. Earlier this year, NASA elevated the leak to the highest level of risk as the rate of air escaping from the module had doubled from one pound of air per day to a little over two pounds.

“While the Russian team continues to search for and seal the leaks, it does not believe catastrophic disintegration of the PrK is realistic,” Bob Cabana, a former NASA astronaut who now chairs the ISS Advisory Committee, said during a meeting on Wednesday, SpaceNews reported. “NASA has expressed concerns about the structural integrity of the PrK and the possibility of a catastrophic failure.”

“The Russians believe that continued operations are safe but they can’t prove to our satisfaction that they are, and the U.S. believes that it’s not safe but we can’t prove to the Russians’ satisfaction that that’s the case,” he added.

Russian teams believe the air leak was likely caused by high cyclic fatigue from micro vibrations, while teams at NASA think pressure and mechanical stress, residual stress, material properties of the module, and environmental exposure are all at play, according to SpaceNews.

The ISS is set for retirement by 2030. [NASA photo]

The air leak was addressed in a recent report by NASA’s Office of Inspector General (OIG), which highlighted its true severity and the risk it poses to the crew. The OIG report stated that the two space agencies can’t seem to agree on the point at which the leak should be considered unsustainable. NASA and Roscosmos met to discuss the ISS air leak, with NASA officials noting that Roscosmos “is confident they will be able to monitor and close the hatch to the Service Module prior to the leak rate reaching an untenable level,” according to the report.

“Although the teams continue to investigate the causal factors for the crack initiation and growth, the U.S. and Russian technical teams don’t have a common understanding of what the likely root cause is or the severity of the consequences of these leaks,” Cabana is quoted in SpaceNews as saying.

The rate of air leaking from the hole increased around a week before the February 14 launch of the Progress MS-26 cargo spacecraft, which docked to the aft end of Zvezda. The hatch that connects the module to the ISS remained open for five days as the crew offloaded the cargo from Progress MS-26 onto the space station, but was closed shut afterwards.

NASA and Roscosmos are currently monitoring the leak and preparing to close the hatch to the service module when access is not required in order to minimize the amount of air lost and isolate the leak itself from the rest of the space station. If required, the space agencies are prepared to permanently shut off the hatch should the leak rate became unmanageable. The ISS would function normally, but there would be one less docking port for spacecraft delivering cargo to the space station.

As the two space agencies continue to discuss the potential risk, the aging space station is inching closer to retirement within the next six years and its hardware may finally be giving in to the wear and tear of the harsh space environment.

[ANS thanks Gizmodo for the above information.]


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Changes to AMSAT-NA TLE Distribution for Nov. 22

Two Line Elements or TLEs, often referred to as Keplerian elements or keps in the amateur community, are the inputs to the SGP4 standard mathematical model of spacecraft orbits used by most amateur tracking programs. Weekly updates are completely adequate for most amateur satellites. TLE bulletin files are updated daily in the first hour of the UTC day. New bulletin files will be posted immediately after reliable elements become available for new amateur satellites. More information may be found at https://www.amsat.org/keplerian-elements-resources/.

XW-2B NORAD Cat ID 40911 Decayed from orbit on 21 November 2024

[ANS thanks Joe Fitzgerald, KM1P, AMSAT Orbital Elements Manager for the above information]


Space Station Raises Orbit Avoiding Orbital Debris

The Progress 89 thrusters were fired at 20:09 UTC on Tuesday, November 19 for 5 minutes, 31 seconds, to raise the orbit of the International Space Station (ISS) to provide an extra margin of distance from a piece of orbital debris from a defunct defense meteorological satellite that broke up in 2015. The Pre-determined Debris Avoidance Maneuver (PDAM) was conducted in coordination with NASA, Roscosmos and the other space station partners.

Without the maneuver, ballistics officials estimated that the fragment could have come within around 2.5 miles of the station.

The maneuver had no impact on station operations and did not affect Thursday’s launch of the Progress 90 cargo craft from the Baikonur Cosmodrome in Kazakhstan.

[Operators attempting to utilize Amateur Radio aboard the ISS should make sure that the Keplerian orbital data in their tracking software has been updated since this change in orbit.]

[ANS thanks NASA for the above information]


ARISS NEWS

Amateurs and others around the world may listen in on contacts between amateurs operating in schools and allowing students to interact with astronauts and cosmonauts aboard the International Space Station. The downlink frequency on which to listen is 145.800 MHz worldwide.

RECENTLY COMPLETED:
Center for the Development of Children and Youth Creativity in the City of Pugachev, Saratov Region, Russia, direct via R4DS
The ISS callsign was RSØISS
The crewmember was Aleksey Ovchinin
The ARISS mentor was RV3DR
Contact was successful Wed 2024-11-20 15:16 UTC
Congratulations to the Center for the Development of Children and Youth Creativity students, Aleksey, mentor RV3DR, and ground station R4DS

Amur State University, Blagoveshchensk, Russia, direct via RКØJ
The ISS callsign was RSØISS
The scheduled crewmember was Alex Gorbunov
The ARISS mentor was RV3DR
Contact was successful Thu 2024-11-21 11:24 UTC
Congratulations to the Amur State University students, Alex, mentor RV3DR, and ground station RКØJ!

Escola Secundária Rafael Bordalo Pinheiro, Caldas da Rainha, Portugal, direct via CS5SS
The ISS callsign was OR4ISS
The scheduled crewmember was Don Pettit, KD5MDT
The ARISS mentor was IKØUSO
Contact was successful: Fri 2024-11-22 16:37:40 UTC 31 deg
Congratulations to the Escola Secundária Rafael Bordalo Pinheiro studnets, Don, mentor IKØUSO, and ground station CS5SS!
Watch for Livestream at https://www.youtube.com/live/QzZOq7bhOas

UPCOMING:
Colégio do Castanheiro, Ponta Delgada, Azores, direct via CQ8CDC
The ISS callsign is presently scheduled to be OR4ISS
The scheduled crewmember is Don Pettit, KD5MDT
The ARISS mentor is IKØUSO
Contact is go for: Tue 2024-11-26 14:57:32 UTC 74 deg
Watch for Livestream at https://www.youtube.com/live/ORRXzIPnjvg

Immanuel Kant Baltic Federal University, Kaliningrad, Russia, direct via TBD
The ISS callsign is presently scheduled to be RSØISS
The scheduled crewmember is Ivan Vagner
The ARISS mentor is RV3DR
Contact is go for: Thu 2024-11-28 15:05 UTC

Scuola Media “Giovanni Verga”, Caltanissetta, Italy, direct via IT9AOI
The ISS callsign is presently scheduled to be OR4ISS
The scheduled crewmember is Don Pettit, KD5MDT
The ARISS mentor is IKØWGF
Contact is go for: Fri 2024-11-29 11:01:30 UTC 59 deg
Watch for Livestream at https://meet.google.com/bdb-hoaf-iaf and also on https://www.youtube.com/@scuolamediafilippocordova

The crossband repeater continues to be ACTIVE (145.990 MHz up {PL 67} & 437.800 MHz down). If any crewmember is so inclined, all they have to do is pick up the microphone, raise the volume up, and talk on the crossband repeater. So give a listen, you just never know.

The packet system is also ACTIVE (145.825 MHz up & down). Ham TV (2395.00 MHz down) is currently STOWED.

As always, if there is an EVA, a docking, or an undocking; the ARISS radios are turned off as part of the safety protocol.

Note, all times are approximate. It is recommended that you do your own orbital prediction or start listening about 10 minutes before the listed time.

The latest information on the operation mode can be found at https://www.ariss.org/current-status-of-iss-stations.html

The latest list of frequencies in use can be found at https://www.ariss.org/contact-the-iss.html

[ANS thanks Charlie Sufana, AJ9N, one of the ARISS operation team mentors for the above information]


Upcoming Satellite Operations

A growing number of satellite rovers are currently engaged in sharing their grid square activations on https://hams.at. By visiting the website, you gain easy access to comprehensive information about the operators responsible for activating specific grid squares. Additionally, you have the ability to assess the match score between yourself and a particular rover for a given pass, while also being able to identify the upcoming satellite passes that are accessible from your location.

+ N4AKV/R plans to operate linear and FM satellites from EM71/EM72 on Nov. 25.
+ ADØHJ is planning his last 2024 rove to the Missouri Ozarks area between December 5th-8th. Mitch has never been to that area so he is looking to do some sightseeing and activate eight new satellite grid squares. EM26-EM28, EM36-EM39, and EN30. He will be working RS-44 passes in the evenings.
See https://hams.at for details.

[ANS thanks hams.at for the above information]


AMSAT Ambassador Activities

AMSAT Ambassadors provide presentations, demonstrate communicating through amateur satellites, and host information tables at club meetings, hamfests, conventions, maker faires, and other events.

February 14-15, 2025
Yuma HAMCON and Southwestern Division Convention
Yuma County Fairgrounds
Yuma, AZ
https://www.yumahamfest.com/
N1UW

[ANS thanks Bo Lowrey, W4FCL, Director – AMSAT Ambassador Program, for the above information]


Satellite Shorts From All Over

+ The space news website Space Daily carried a full article on Nov. 12 about the 50th anniversary of the launch of amateur radio satellite AO-7. As noted in anniversary articles by Frank Karnauskas, N1UW, AMSAT Vice President – Development, that have been published here in the AMSAT News Service bulletins [see above for this week’s installment], AO-7 is the world’s oldest active satellite. The Space Daily article, by reporter Clarence Oxford, incorporated a good share of Frank’s text from ANS issue #308 published on Nov. 3. (ANS thanks Space Daily for the above information.)

+ The Space Force wants its next fleet of GPS satellites to be smaller, cheaper and more resilient — and it’s looking to a mix of commercial and defense firms to help design those spacecraft. The program, expected to cost $1 billion over the next five years, comes amid growing concern from Pentagon and other government leaders about GPS vulnerability. The system, which guides weapons and helps military units navigate, has been a target for Russia in its war with Ukraine, using electronic warfare to jam signals on a regular basis. Users have also reported increased spoofing incidents, a method of manipulating GPS data to confuse a receiver about its location. A larger number of small satellites should make it harder for enemies to target the fleet and will ensure there’s a backup capability when they do, the Space Force says. (ANS thanks Defense News for the above information.)

+ Earlier this month, three tiny Australian satellites from Curtin University’s Binar Space Program burned up in Earth’s atmosphere. That was always going to happen. In fact, Binar means “fireball” in the Noongar language of the First Nations people of Perth. But these CubeSats, known as Binar-2, 3, and 4, entered the atmosphere much sooner than originally planned. They only lasted for two months – a third of what was expected. Recent high solar activity has been causing an unexpected headache for satellite operators in the last few years, and it’s only increasing. (ANS thanks Science Alert for the above information.)

+ China has taken another step toward its crewed lunar goals by successfully testing fairing separation for its Long March 10 moon rocket series. The fairing separation test was conducted recently, according to a Nov. 20 statement from the China Academy of Launch Vehicle Technology (CALT). The separation test is one of a number of milestones needed in order to get the Long March 10 ready for flight, with a first launch to low earth orbit currently targeted for 2026. China has committed to the goal of getting a pair of its astronauts onto the lunar surface by 2030. (ANS thanks Space News for the above information.]


Join AMSAT today at https://launch.amsat.org/

In addition to regular membership, AMSAT offers membership to:

* Societies (a recognized group, clubs or organization).
* Primary and secondary school students are eligible for membership at one-half the standard yearly rate.
* Post-secondary school students enrolled in at least half time status shall be eligible for the student rate for a maximum of 6 post-secondary years in this status.
* Memberships are available for annual and lifetime terms.

Contact info [at] amsat.org for additional membership information.

73 and remember to help Keep Amateur Radio in Space!

This week’s ANS Editor, Mark Johns, KØJM
mjohns [at] amsat.org