mardi 17 août 2021

Zhurong completes its designed mission

 







CNSA - Tianwen-1 (天問-1) Mission to Mars logo.


August 17, 2021

Utopia Planitia seen by Zhurong

According to CNSA, the Tianwen-1 rover “Zhurong” successfully completed the designed exploration mission. As of 15 August 2021, Zhurong has operated on the surface of Mars for 90 Martian days (approximately 92 Earth days) and traveled 889 meters in total.

Zhurong completes its designed mission

All scientific payloads were started for detection, and a total of about 10GB of raw data was obtained. Zhurong is reported to be in good condition and will continue to drive towards the ancient sea-land interface in the southern part of Utopia Planitia. Tianwen-1 (天问一号) is China’s first Mars exploration mission with an orbiter, a lander and a rover named Zhurong (祝融).

Related articles:

Tianwen-1 and Zhurong – a new phase of Mars exploration
https://orbiterchspacenews.blogspot.com/2021/08/tianwen-1-and-zhurong-new-phase-of-mars.html

Tianwen-1 Mission to Mars - Close-Up of Zhurong’s Parachute
https://orbiterchspacenews.blogspot.com/2021/07/tianwen-1-mission-to-mars-close-up-of.html

Tianwen-1 Mission to Mars - New images from Zhurong
https://orbiterchspacenews.blogspot.com/2021/07/tianwen-1-mission-to-mars-new-images.html

Zhurong landing on Mars & Sounds of Zhurong’s descend onto Mars
https://orbiterchspacenews.blogspot.com/2021/06/zhurong-landing-on-mars-sounds-of.html

Zhurong rover and Tianwen-1 lander on Mars
https://orbiterchspacenews.blogspot.com/2021/06/zhurong-rover-and-tianwen-1-lander-on.html

Tianwen-1 Lander and Zhurong Rover seen by NASA’s Mars Reconnaissance Orbiter
https://orbiterchspacenews.blogspot.com/2021/06/tianwen-1-lander-and-zhurong-rover-seen.html

Zhurong is roving on Mars!
https://orbiterchspacenews.blogspot.com/2021/05/zhurong-is-roving-on-mars.html

Why the China Mars rover’s landing site has geologists excited & Zhurong’s first images from Mars
https://orbiterchspacenews.blogspot.com/2021/05/why-china-mars-rovers-landing-site-has.html

Tianwen-1 orbiter relays Zhurong rover’s data and images
https://orbiterchspacenews.blogspot.com/2021/05/tianwen-1-orbiter-relays-zhurong-rovers.html

Zhurong landed on Mars! The Tianwen-1 rover is on Utopia Planitia (Videos)
https://orbiterchspacenews.blogspot.com/2021/05/zhurong-landed-on-mars-tianwen-1-rover.html

China succeeds in landing its rover on Mars
https://orbiterchspacenews.blogspot.com/2021/05/china-succeeds-in-landing-its-rover-on.html

Related link:

For more information about China National Space Administration (CNSA), visit: http://www.cnsa.gov.cn/

Image, Video, Text, Credits: China Central Television (CCTV)/China National Space Administration (CNSA)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

China Space Station - Shenzhou-12 crew prepares for second spacewalk

 







China Manned Space logo.


August 17, 2021

Shenzhou-12 crew prepares for second spacewalk

The Shenzhou-12 crew, astronauts Nie Haisheng (commander), Liu Boming and Tang Hongbo,  prepares for the second extravehicular activity (EVA or spacewalk) planned during their three months mission on the Tianhe core module (天和核心舱), the first and main component of the China Space Station (中国空间站), informally known as Tiangong (天宫, Heavenly Palace).

Shenzhou-12 crew prepares for second spacewalk

During the last 30 days, the Shenzhou-12 (神舟十二号) astronauts “activated the magnetic levitation experiment facility” that “includes a chamber of high-level micro-gravity”, “completed assembly of a space centrifuge, an equipment used for centrifugalizing samples”, and performed some “spring cleaning” in the Tianhe core module.

Related articles:

China Space Station - Shenzhou-12 astronauts test their health
https://orbiterchspacenews.blogspot.com/2021/08/china-space-station-shenzhou-12.html

CMS - Shenzhou-12 - one month on board the China Space Station
https://orbiterchspacenews.blogspot.com/2021/07/cms-shenzhou-12-one-month-on-board.html

First spacewalk on the China Space Station
https://orbiterchspacenews.blogspot.com/2021/07/first-spacewalk-on-china-space-station.html

China Space Station - The Tianhe core module has Hall-effect thrusters - CSS astronauts unpack EVA spacesuit
https://orbiterchspacenews.blogspot.com/2021/06/china-space-station-tianhe-core-module.html

China Space Station - Shenzhou-12 crew begins three-month mission
https://orbiterchspacenews.blogspot.com/2021/06/china-space-station-shenzhou-12-crew.html

China sends its first crew to its Space Station
https://orbiterchspacenews.blogspot.com/2021/06/china-sends-its-first-crew-to-its-space.html

Long March-7 Y3 launches Tianzhou-2 & Tianzhou-2 docking to the Tianhe Core Module
https://orbiterchspacenews.blogspot.com/2021/05/long-march-7-y3-launches-tianzhou-2.html

Tianhe completes in-orbit checks & Long March-7 Y3 ready to launch Tianzhou-2
https://orbiterchspacenews.blogspot.com/2021/05/tianhe-completes-in-orbit-checks-long.html

China Space Station
https://orbiterchspacenews.blogspot.com/2021/05/china-space-station.html

CASC - Long March-5B Y2 launches the Tianhe Core Module
https://orbiterchspacenews.blogspot.com/2021/04/casc-long-march-5b-y2-launches-tianhe.html

Related link:

For more information about China National Space Administration (CNSA), visit: http://www.cnsa.gov.cn/

Image, Video, Text, Credits: China Central Television (CCTV)/China National Space Administration (CNSA)/SciNews/Orbiter.ch Aerospace/Roland Berga.

Greetings, Orbiter.ch

Vega launches Pléiades Neo and CubeSats

 







ESA - Radcube 2021 Mission patch.


August 17, 2021

Europe’s Vega has delivered Pléiades Neo-4 and four auxiliary payloads, SunStorm, RadCube and LEDSAT developed through ESA, and BRO-4, to their planned orbits.

Vega liftoff on flight VV19

Liftoff of flight VV19 from Europe’s Spaceport in French Guiana came at 02:47 BST on 17 August (03:47 CEST; 22:47 local time on 16 August) for a mission lasting about 105 minutes.

Pléiades Neo-4, the primary payload with a launch mass of 922 kg, was the first to be released into a Sun-synchronous orbit about 55 minutes into the mission.

Then, following two burns interrupted by a ballistic phase lasting 41 minutes, Vega’s upper stage released four auxilliary payloads in a coordinated sequence.

To comply with debris regulations to help keep space clean, the upper stage burned a final time to deorbit itself to ensure direct reentry and burn up high in the atmosphere over the ocean.

Vega launches Pléiades Neo 4

Pléiades Neo-4 is an Earth observation satellite owned and operated by Airbus Defence and Space. It is the second of a constellation of four satellites to provide very high-resolution images of Earth’s surface several times per day to a 30 cm per-pixel resolution. This data will be used to monitor the effects of climate change, for mapping, in defence, and will offer near-real time emergency service response capabilities over the next 10 years. Pléiades Neo-4 joins Pléiades Neo-3 which was launched on Vega’s first launch this year.

Sharing this launch were three CubeSats from ESA: SunStorm, RadCube and LEDSAT.

This SunStorm CubeSat is being used to demonstrate miniaturised space weather instruments

SunStorm and RadCube will demonstrate miniaturised space weather instruments for use in later operational space weather missions and have been developed through ESA’s General Support Technology Programme (GSTP).

SunStorm, a two-unit CubeSat built and operated by Reaktor Space Lab in Finland, hosts a new solar X-ray flux monitor which will detect coronal mass ejections from the Sun which threaten satellites and terrestrial power and communications networks. It demonstrates a novel ant-sized silicon drift detector, developed by Isaware in Finland, a technology planned to be used on the ESA Lagrange space weather mission.

RadCube demonstrates miniaturised space weather instruments

RadCube is a three-unit CubeSat built through a collaboration led by C3S in Hungary. It will demonstrate a new CubeSat platform from C3S and a new space weather in-situ monitoring instrument called RagMag. The instrument consists of a radiation telescope developed by the Centre for Energy Research in Hungary, and a magnetometer developed by Imperial College London in UK, which is to be deployed on the end of a boom system developed by Astronika in Poland. It carries an experiment to show how radiation in space damages electronics, which will lead to safer components and spacecraft.

Members of the LEDSAT team in the cleanroom

LEDSAT is a student project from La Sapienza, University of Rome, Italy, supported by the ESA Education Office via the Fly Your Satellite! programme. LEDSAT is covered with 140 Light Emitting Diodes (LED) which can light up when it is not illuminated by the Sun. This enables extended optical tracking of satellite position, attitude and velocity by ground-based telescopes, and will be used to perform preliminary tests on optical communications.

In addition, BRO-4 (Breizh Reconnaissance Orbiter) is one of a constellation of satellites developed by French startup company, UnSeenLabs. BRO-4, is a shoebox-sized spectrum monitoring and electromagnetic intelligence service for maritime and aerial traffic surveillance. A planned constellation by 2025 will comprise 20–25 nanosatellites.

Vega has been in operation since 2012 and is ideal for launching light satellites to multiple orbits in a single launch. It is a 3 m-diameter single-body vehicle comprising four stages. It stands 30 m tall with a liftoff mass of 137 tonnes. The total payload mass for this launch was about 1029 kg.

“We celebrate another Vega success while we gear up for the transition to the enhanced Vega-C version and prepare future evolutions of this launch system beyond 2025. We’re progressing on all these fronts in parallel. Vega is and will remain an essential element of European space transportation logistics,” commented Daniel Neuenschwander, ESA Director of Space Transportation.

Related links:

Space Transportation: https://www.esa.int/Enabling_Support/Space_Transportation

Vega: https://www.esa.int/Enabling_Support/Space_Transportation/Vega

Images, Video, Text, Credits: ESA/CNES/Arianespace/LEDSAT team/SciNews.

Best regards, Orbiter.ch

Why NASA’s Mars rover failed to collect its first rock core

 







NASA - Mars 2020 Perseverance Rover logo.


August 17, 2021

Intriguing rocks turned out to be too crumbly for Perseverance to drill successfully. It’s moving on to try elsewhere.


Image above: This composite image of the Perseverance rover’s first borehole (2.7 centimetres wide) suggests that the rock sample was probably pulverized. Image Credits: NASA/JPL-Caltech/MSSS.

After drilling into its first rock on Mars but failing to capture it in a storage tube on 6 August, NASA’s Perseverance rover is rolling onwards. Rather than make a second attempt now at drilling in the same geologically interesting area in Mars’s Jezero Crater, it will instead drill into different terrain next month, in the hope that those rocks will be more amenable to coring.

After a few days assessing what went wrong during the first attempt, NASA announced on 11 August that the rover had pulverized the sampled rock into powder and small fragments. They fell to the crater floor rather than sliding into the tube, as an intact core would have done.

“It took a few minutes for this reality to sink in,” wrote Louise Jandura, the chief engineer for sampling and caching at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, which operates the rover, in an 11 August update.

Perseverance is attempting to become the first mission to drill and collect a suite of rock cores from the Martian surface. It is planned that other spacecraft will eventually retrieve the samples and bring them back to Earth, where scientists can study them. “This is just another reminder that there are still a lot of unknowns about Mars,” says Meenakshi Wadhwa, a planetary scientist at Arizona State University in Tempe who is NASA’s principal scientist for the sample-retrieval effort. “This planet still has the capacity to surprise us when we least expect it.”

Mars Perseverance Rover sampling operation. Animation Credits: NASA/JPL-Caltech

Researchers were particularly excited about the rover’s first drilling attempt. They had selected one of the flat rocks that make up much of the floor of Jezero Crater, where the rover landed in February, and which it has been exploring since then. Preliminary exploration of those flat rocks — dubbed the ‘cratered floor fractured rough’ — suggested that they might be volcanic in origin, perhaps even from an ancient lava flow. Collecting a volcanic rock from Mars and returning it to Earth would allow geologists to date its formation precisely, and thus pin down a chronology for much of Mars’s geological history.

But despite initial images suggesting that Perseverance had successfully drilled 7 centimetres into the surface and extracted a slim cylinder of intact rock, NASA later discovered that the sampling tube that had been automatically sealed and stored inside the rover’s belly was empty.

The rock was crumblier than engineers had expected, says Jennifer Trosper, the mission’s project manager at the JPL. Perhaps there was a hard layer of rock hiding looser material beneath it, or perhaps there were large voids in the rock that caused it to collapse. “There wasn’t anything obvious,” she says, to suggest “that this might disintegrate or be pulverized when we cored it”.

Taking a step back

Rather than try again with the cratered floor fractured rough, Perseverance has already departed the area and is heading towards a region named South Séítah, which probably contains layered sedimentary rocks that are more like the Earth rocks that engineers drilled during tests before the mission’s launch. “We are going to step back and do something we are more confident of,” says Trosper. The rover will try to drill a core there, perhaps in early September. When it does, engineers will pause the automated drilling process to check whether a core has been extracted before the rover takes the next steps of sealing the tube and storing it away.


Image above: Perseverance touched down on Mars in February at the Octavia E. Butler Landing Site in Jezero Crater. It attempted to collect its first rock core from flat stones that engineers have dubbed cratered floor fractured rough (Cr-Fr). Next, it will try to drill again in a sandy area called Séítah, before reversing direction (following the yellow dashed path) and heading towards Jezero’s ancient delta (labelled Three Forks). Image Credits: NASA/JPL-Caltech/University of Arizona.

The empty tube it stored on 6 August will serve as a sample of the Martian atmosphere, which the Perseverance team intended to collect at some point during the mission, although not so soon. The rover carries 43 sampling tubes, so 42 remain. The ultimate goal is to fill about 35 tubes with Martian rock and soil, from various parts of Jezero Crater. They would return to Earth no earlier than 2031.

Engineers tested the Perseverance drilling system more than 100 times on a range of rocks on Earth, to prepare for everything the rover might encounter on Mars. But the cratered floor fractured rough proved beyond the system’s experience.

Perseverance isn’t the first spacecraft to run into problems with Mars rock and soil. NASA’s InSight lander deployed a probe known as the mole, which tried for nearly two years to bury itself up to 5 metres deep in the Martian soil to measure heat flow. The team finally gave up in January, after the probe was unable to build up enough friction against the soil to hammer itself into the ground. And NASA’s Curiosity rover, which has been exploring Gale Crater since 2012, has occasionally and unexpectedly broken rocks apart while drilling into them.

Curiosity and Perseverance are similar in many respects — Perseverance was actually built using much of the leftover hardware from Curiosity — but there is one major difference in how they drill into the Martian surface. Curiosity intentionally grinds rock into powder, which it then places inside onboard analytical instruments for scientific studies. NASA designed Perseverance to extract intact cores that slide into its sampling tubes. So crumbly rocks are good for Curiosity, but not for Perseverance.

‘We’ll figure it out’

After its second attempt to collect a core, at South Séítah, Perseverance will head back in the direction it came from, once again crossing the cratered floor fractured rough — which it might try sampling again if the engineering team can find a more promising drilling site, with rocks that look like they will hold together better. “Anomalies like this are what we’re created to solve,” says Trosper. “I’m a little disappointed, but I think we’ll figure it out.”

Perseverance will then loop around a region of sand dunes on its way to its ultimate destination, an ancient river delta in Jezero that might contain traces of Martian life.

doi: https://doi.org/10.1038/d41586-021-02208-z

More About Perseverance

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith.

Subsequent NASA missions, in cooperation with ESA (European Space Agency), would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance:

https://mars.nasa.gov/mars2020/ and https://nasa.gov/perseverance

Related article:

NASA’s Perseverance Team Assessing First Mars Sampling Attempt
https://orbiterchspacenews.blogspot.com/2021/08/nasas-perseverance-team-assessing-first.html

Images (mentioned), Animation (mentioned), Text, Credits: Nature/Alexandra Witze/NASA/JPL-Caltech.

Greetings, Orbiter.ch

lundi 16 août 2021

Week Kicks Off with Spacewalk Preps, Cygnus Cargo Transfers

 







ISS - Expedition 65 Mission patch.


August 16, 2021

Two astronauts and two cosmonauts are gearing up for three spacewalks set to begin next week at the International Space Station. The Expedition 65 crew is also continuing to unpack a U.S. cargo craft in the middle of ongoing science and maintenance activities.

The first spacewalk is planned to take place on Aug. 24. Commander Akihiko Hoshide and Flight Engineer Mark Vande Hei will exit the Quest airlock in their U.S. spacesuits around 8 a.m. EDT and translate over to the Port-4 truss structure. Once there, the duo will prepare the worksite for the next set of Roll-Out Solar Arrays due to arrive on an upcoming SpaceX Cargo Dragon mission. The pair went over their spacewalk maneuvers on a computer Monday afternoon.


Image above: The SpaceX Falcon 9 rocket with the Dragon capsule atop is raised to the vertical position on June 2, 2021, at Launch Complex 39A at NASA’s Kennedy Space Center in Florida, in preparation for the company’s 22nd Commercial Resupply Services mission for NASA to the International Space Station. NASA and SpaceX are targeting Saturday, Aug. 28, at 3:37 a.m. EDT, for launch of the 23rd commercial resupply services mission. Image Credit: SpaceX.

Cosmonauts Oleg Novitskiy and Pyotr Dubrov will perform the other two spacewalks in early September to prepare cables and other external equipment for the recently arrived Nauka Multipurpose Laboratory Module. Today, the flight engineers from Roscosmos reviewed the steps and procedures planned for the second spacewalk.

NASA Flight Engineers Megan McArthur and Shane Kimbrough joined ESA (European Space Agency) Flight Engineer Thomas Pesquet and took turns offloading cargo packed inside the Cygnus space freighter today. Cygnus delivered over four tons of cargo including over 2,300 pounds of new science experiments last week. The resupply ship from Northrop Grumman will stay attached to the Unity module for about three months.


Image above: Russia’s Soyuz MS-18 crew ship (foreground) and Nauka Multipurpose Laboratory Module are pictured docked to the station as it orbited above Africa’s Indian Ocean coast. Image Credit: NASA.

Science is still ongoing at the orbital lab as Vande Hei swapped fuel bottles inside the Combustion Integrated Rack and set up a sample for the Ring Sheared Drop fluid physics study. Hoshide serviced samples in a microscope for a biology study observing how cells sense gravity then installed the Kaber small satellite deployer inside the Kibo laboratory module.

Related article:

NASA Announces Date for SpaceX’s 23rd Cargo Resupply Mission
https://www.nasa.gov/press-release/nasa-announces-date-for-spacex-s-23rd-cargo-resupply-mission

Related links:

Expedition 65: https://www.nasa.gov/mission_pages/station/expeditions/expedition65/index.html

Port-4 truss structure: https://www.nasa.gov/mission_pages/station/structure/elements/truss-structure

Unity module: https://www.nasa.gov/mission_pages/station/structure/elements/unity

Combustion Integrated Rack: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=317

Ring Sheared Drop: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7383

How cells sense gravity: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8029

Kaber small satellite deployer: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=1788

Kibo laboratory module: https://www.nasa.gov/mission_pages/station/structure/elements/japan-kibo-laboratory

Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/overview.html

International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html

Images (mentioned), Text, Credits: NASA/Mark Garcia.

Greetings, Orbiter.ch

Star Formation in the Constellation of Gemini, the Twins

 







NASA - Hubble Space Telescope patch.


Aug 16, 2021


Nestled among the vast clouds of star-forming regions like this one lie potential clues about the formation of our own solar system.

This image from the NASA/ESA Hubble Space Telescope features AFGL 5180, a beautiful stellar nursery located in the constellation of Gemini (the Twins).

At the center of the image, a massive star is forming and blasting cavities through the clouds with a pair of powerful jets, extending to the top right and bottom left of the image. Light from this star is mostly escaping and reaching us by illuminating these cavities, like a lighthouse beacon piercing the storm clouds.

Stars are born in dusty environments and although this dust makes for spectacular images, it can prevent astronomers from seeing stars embedded in it. Hubble’s Wide Field Camera 3 (WFC3) instrument is designed to capture detailed images in both visible and infrared light, meaning that the young stars hidden in vast star-forming regions like AFGL 5180 can be seen much more clearly.

For more information about Hubble, visit:

http://hubblesite.org/

http://www.nasa.gov/hubble

http://www.spacetelescope.org/

Image Credits: ESA/Hubble & NASA, J. C. Tan (Chalmers University & University of Virginia), R. Fedriani (Chalmers University); Acknowledgment: Judy Schmidt
Text Credit: European Space Agency (ESA).

Best regards, Orbiter.ch

Fizzing Sodium Could Explain Asteroid Phaethon’s Cometlike Activity

 







NASA - Jet Propulsion Laboratory logo.


Aug 16, 2021

Models and lab tests suggest the asteroid could be venting sodium vapor as it orbits close to the Sun, explaining its increase in brightness.


Image above: This illustration depicts asteroid Phaethon being heated by the Sun. The asteroid’s surface gets so hot that sodium inside Phaethon’s rock may vaporize and vent into space, causing it to brighten like a comet and dislodge small pieces of rocky debris. Image Credits: NASA/JPL-Caltech/IPAC.

As a comet zooms through the inner solar system, the Sun heats it, causing ices below the surface to vaporize into space. The venting vapor dislodges dust and rock, and the gas creates a bright tail that can extend millions of miles from the nucleus like an ethereal veil.

Whereas comets contain lots of different ices, asteroids are mainly rock and not known for producing such majestic displays. But a new study examines how near-Earth asteroid Phaethon may in fact exhibit cometlike activity, despite lacking significant quantities of ice.

Known to be the source of the annual Geminid meteor shower, the 3.6-mile-wide (5.8 kilometer-wide) asteroid brightens as it gets close to the Sun. Comets typically behave like this: When they heat up, their icy surfaces vaporize, causing them to become more active and brighten as the venting gases and dust scatter more sunlight. But what is causing Phaethon to brighten if not vaporizing ices?

The culprit could be sodium. As the new study’s authors explain, Phaethon’s elongated, 524-day orbit takes the object well within the orbit of Mercury, during which time the Sun heats the asteroid’s surface up to about 1,390 degrees Fahrenheit (750 degrees Celsius). With such a warm orbit, any water, carbon dioxide, or carbon monoxide ice near the asteroid’s surface would have been baked off long ago. But at that temperature, sodium may be fizzing from the asteroid’s rock and into space.

“Phaethon is a curious object that gets active as it approaches the Sun,” said study lead Joseph Masiero, a scientist at IPAC, a research organization at Caltech. “We know it’s an asteroid and the source of the Geminids. But it contains little to no ice, so we were intrigued by the possibility that sodium, which is relatively plentiful in asteroids, could be the element driving this activity.”

Asteroid-Meteor Connection

Masiero and his team were inspired by observations of the Geminids. When meteoroids – small pieces of rocky debris from space – streak through Earth’s atmosphere as meteors, they disintegrate. But before they do, friction with the atmosphere causes the air surrounding the meteoroids to reach thousands of degrees, generating light. The color of this light represents the elements they contain. Sodium, for example, creates an orange tinge. The Geminids are known to be low in sodium.

Until now, it was assumed that these small pieces of rock somehow lost their sodium after leaving the asteroid. This new study suggests that the sodium may actually play a key role in ejecting the Geminid meteoroids from Phaethon’s surface.  

The researchers think that as the asteroid approaches the Sun, its sodium heats up and vaporizes. This process would have depleted the surface of sodium long ago, but sodium within the asteroid still heats up, vaporizes, and fizzes into space through cracks and fissures in Phaethon’s outermost crust. These jets would provide enough oomph to eject the rocky debris off its surface. So the fizzing sodium could explain not only the asteroid’s cometlike brightening, but also how the Geminid meteoroids would be ejected from the asteroid and why they contain little sodium.

“Asteroids like Phaethon have very weak gravity, so it doesn’t take a lot of force to kick debris from the surface or dislodge rock from a fracture,” said Björn Davidsson, a scientist at NASA’s Jet Propulsion Laboratory in Southern California and a co-author of the study. “Our models suggest that very small quantities of sodium are all that’s needed to do this – nothing explosive, like the erupting vapor from an icy comet’s surface; it’s more of a steady fizz.”

Lab Tests Required

To find out if sodium turns to vapor and vents from an asteroid’s rock, the researchers tested samples of the Allende meteorite, which fell over Mexico in 1969, in a lab at JPL. The meteorite may have come from an asteroid comparable to Phaethon and belongs to a class of meteorites, called carbonaceous chondrites, that formed during the earliest days of the solar system. The researchers then heated chips of the meteorite to the highest temperature Phaethon would experience as it approaches the Sun.

“This temperature happens to be around the point that sodium escapes from its rocky components,” said Yang Liu, a scientist at JPL and a study co-author. “So we simulated this heating effect over the course of a ‘day’ on Phaethon – its three-hour rotation period – and, on comparing the samples’ minerals before and after our lab tests, the sodium was lost, while the other elements were left behind. This suggests that the same may be happening on Phaethon and seems to agree with the results of our models.”

The new study supports a growing body of evidence that categorizing small objects in our solar system as “asteroids” and “comets” is oversimplified, depending not only on how much ice they contain, but also what elements vaporize at higher temperatures.

“Our latest finding is that if the conditions are right, sodium may explain the nature of some active asteroids, making the spectrum between asteroids and comets even more complex than we previously realized,” said Masiero.

The study, titled “Volatility of Sodium in Carbonaceous Chondrites at Temperatures Consistent with Low-Perihelia Asteroids,” was published in The Planetary Science Journal on Aug. 16, 2021.

Related links:

The Planetary Science Journal: https://doi.org/10.3847/PSJ/ac0d02

IPAC: https://www.ipac.caltech.edu/

Asteroids: https://www.nasa.gov/mission_pages/asteroids/main/index.html

Comets: http://www.nasa.gov/comets

Meteors & Meteorites: http://www.nasa.gov/topics/solarsystem/features/watchtheskies/index.html

Image (mentioned), Text, Credits: NASA/Tony Greicius/Josh Handal/Karen Fox/JPL/Ian J. O’Neill.

Greetings, Orbiter.ch