Tag: Mars

InSight detects additional 3+ magnitude quakes on Mars

8:23 am

Martian quake map as seen by InSight

According to a JPL press release today, the seismometer on the Mars lander InSight detected two new 3+ magnitude quakes in March, both coming from the Cerberus Fossae region, the same region where the bulk of seismic activity has so far been pinpointed on Mars.

The map to the right was presented several weeks ago at the 52nd Lunar and Planetary conference, and could possibly include one of these two new quakes. The timing however of these March quakes is significant:

The new quakes have something else in common with InSight’s previous top seismic events, which occurred almost a full Martian year (two Earth years) ago: They occurred in the Martian northern summer. Scientists had predicted this would again be an ideal time to listen for quakes because winds would become calmer. The seismometer, called the Seismic Experiment for Interior Structure (SEIS), is sensitive enough that, even while it is covered by a dome-shaped shield to block it from wind and keep it from getting too cold, wind still causes enough vibration to obscure some marsquakes. During the past northern winter season, InSight couldn’t detect any quakes at all.

They are beginning to use the lander’s scoop to cover the seismometer and its communications tether with sand to protect both from the wind and temperature fluctuations. Once done they hope to be able to detect quakes during the entire Martian year, though this ability will be further limited by a reduction in power.

Despite the winds that have been shaking the seismometer, InSight’s solar panels remain covered with dust, and power is running lower as Mars moves away from the Sun. Energy levels are expected to improve after July, when the planet begins to approach the Sun again. Until then, the mission will successively turn off the lander’s instruments so that InSight can hibernate, waking periodically to check its health and communicate with Earth. The team hopes to keep the seismometer on for another month or two before it has to be temporarily turned off.

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Tianwen-1’s engineers set mid-May for rover landing on Mars

7:59 am

The new colonial movement: The science team for China’s Tianwen-1 orbiter are now targeting mid-May for when they will release and land the as-yet unnamed rover for its landing on Mars.

Wang Chi, director of the National Space Science Center at the Chinese Academy of Sciences, said March 23 that Tianwen 1’s lander and rover are scheduled to touch down on Mars in May.

“The first Chinese Mars mission, Tianwen 1, is now orbiting Mars, and we are landing in the middle of May,” Wang said in a presentation to the National Academies’ Space Studies Board. “We are open to international cooperation, and the data will be available publicly soon.” [emphasis mine]

Though China has generally released the scientific data of its lunar probes eventually, they have done it slowly. In the case of Tianwen-1, they released so far practically nothing, with the only images released being two hi-resolution ground images and a handful of distant global pictures of Mars.

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Very peculiar flow features on Mars

12:29 pm

Peculiar flows on Mars
Click for full image.

Today’s cool image focuses on one of the weirdest flow features I have yet seen on Mars. The first photo to the right, rotated and cropped to post here, comes from a January 27, 2021 picture by the high resolution camera on Mars Reconnaissance Orbiter (MRO). This cropped section focuses on the middle of three such weird features, two close flows heading downhill on the interior rim of very eroded 28-mile-wide crater. For some reason the flows also have depressions on their crowns. The depressions almost look like someone carved them out with a spackling spatula. In fact, the MRO science team agrees, labeling this image as “Spatulate Depressions with and without Upslope Gullies.”

The second image to the right shows a wider crop of the same picture, and explains the reason for the last half of that label.
» Read more

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Ingenuity unfolded and ready for placement on ground

9:59 am

Ingenuity unfolded
Click for full image.

The photo to the right, taken yesterday, shows Perseverance’s Ingenuity helicopter now vertical with its legs deployed, hanging from the bottom of the rover and ready for placement on the ground.

The next step will be drop Ingenuity those last few inches. Once released Perseverance will quickly drive away, as it will no longer be providing power to the helicopter and will instead be blocking its solar panels from sunlight.

Perseverance will then proceed to its lookout post while engineers check out Ingenuity to make sure all is working.

The targeted flight date remains April 8th.

UPDATE: JPL just announced that it is delaying Ingenuity’s flight to April 11th. The announcement was done by a tweet, so provided no explanation as to why JPL decided to delay three days.

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Ice under Mars’ biggest volcanic ash field, at the equator?

11:24 am

Wind eddies on Mars
Click for full image.

According to new data obtained from the radar instruments on Mars Reconnaissance Orbiter (MRO) and Mars Express, scientists now think that the Medusae Fossae Formation, Mars’ biggest volcanic ash field and thought by some to be the source of most of the planet’s dust, might have an underground layer of ash that is also ice-rich. From their abstract:

The Medusae Fossae Formation (MFF) on Mars covers a vast area along the boundary between the rugged southern highlands and the smooth northern plains. While the MFF appears to be thick sediments or volcanic ash slowly eroding in the martian winds, how this material was emplaced remains mysterious. Most intriguing is evidence suggesting that some areas of the MFF may contain water ice. In this work we use sounding radar data from the SHARAD instrument on the Mars Reconnaissance Orbiter to probe up to 600 m below the surface and measure the electrical properties of the MFF material. The results suggest that the shallow parts of the MFF deposits are very porous and compress readily under their own weight. To match deeper probing by the Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument on Mars Express requires a second layer of either vast porous deposits or ice‐rich material protected from sublimation by the dry sediments.

The MRO image above, originally posted here in November 2020, shows one example of the typical wind erosion found in the Medusae ash field. Apparently the ground-penetrating radar from orbit now suggests the possibility that there is an ash layer rich in ice, at depths beginning somewhere between 1,000 to 2,000 feet below the surface.
» Read more

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Al-Amal reaches science orbit

1:22 pm

Cerberus Fossae, as seen by Al-Amal
Click for full image.

Elysium Mons and Cereberus Fossae

The new colonial movement: The United Arab Emirates (UAE) Al-Amal (Hope) Mars Orbiter has now reached its science orbit, and will begin its two years of observations (one full Martian year) of the Martian atmosphere on April 14th.

The photo to the right, cropped to post here, is part of a much larger image covering a good portion of the 600-mile-long fissures dubbed Cerberus Fossae and located Elysium Planitia, the vast lava plains located between the giant volcanoes Elysium and Olympus Mons, where most of the Martian quakes have so-far been detected by InSight. The context map below provides a wider context (the red boxes indicating high resolution Mars Reconnaissance Orbiter images). I think the area covered by this section of Al-Amal’s picture is near the western end of Cerberus Fossae.

The image was posted today in the image gallery for Al-Amal. Unfortunately there is no separate webpage for this particular post, so that link will take a long time to load, as apparently all the images there are large, not thumbnails. From their text:

On 15 March 2021, the Emirates eXploration Imager (EXI) captured a monochromatic image of the Cerberus Fossae, a fracture system that stretches for more than 1,000 km across the Martian surface, with a spatial scale of approximately 180 meters/pixel. The Emirates Mars Mission transitioned from the capture orbit to its science orbit with the successful completion of a 510-second burn of its thrusters. The Hope Probe is now in its final orbit of Mars and ready for its two-year science data gathering – the core aim of the mission. The science phase will commence on 14 April 2021.

The goal of Al-Amal is to study the atmosphere. This camera will provide wide shots, mostly for the purpose of observing the coming and going of cloud features. Nonetheless, this is a nice wide view of Mars.

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NASA in contact with China to get the orbital data of its Tianwen-1 Mars Orbiter

10:20 am

Though by law NASA and the scientists cannot exchange data or communications with China due to security concerns, NASA and Chinese officials did exchange communications recently in order to coordinate the orbits of their orbiters presently circling Mars.

Jurczyk noted that NASA’s knowledge of China’s space program is largely limited to publicly available information because of restrictions placed by federal law on its interactions with Chinese organizations. Those restrictions do allow NASA to engage with China if approved by Congress. “Most recently, we had an exchange with them on them providing their orbital data, their ephemeris data, for their Tianwen-1 Mars orbiting mission, so we could do conjunction analysis around Mars with the orbiters,” he said.

In a brief statement to SpaceNews late March 29, NASA confirmed it exchanged information with the China National Space Administration (CNSA), as well as other space agencies that operate spacecraft at Mars. “To assure the safety of our respective missions, NASA is coordinating with the UAE, European Space Agency, Indian Space Research Organisation and the China National Space Administration, all of which have spacecraft in orbit around Mars, to exchange information on our respective Mars missions to ensure the safety of our respective spacecraft,” the agency said. “This limited exchange of information is consistent with customary good practices used to ensure effective communication among satellite operators and spacecraft safety in orbit.”

Such limited communications are actually permitted under the law that Congress passed, as long as they do not involve any exchange of technical information. There has been a push, however, in the planetary community for years to increase direct communications with China, allowing the transfer of all kinds of information, both scientific and technical. Until the law gets changed none of this should happen.

Of course, what matters laws these days? I will not be surprised if the Biden administration, rather than demanding a change in the law, instead begins expanded communications between NASA and China, in complete and utter contempt for the law, with no one objecting.

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Martian glaciers flowing off interior walls of Renaudot Crater

12:57 pm

Overview map

Cool image time! In the March 1st image release from the high resolution camera on Mars Reconnaissance Orbiter (MRO) were two pictures covering sections of the interior rim of 40-mile-wide Renaudot Crater, located in the northern lowland plains of Mars north of the region I dub Mars’ glacier country.

The map to the right provides the context. The two red boxes in Renaudot Crater show the location of the two images below, with the first being the one to the left. Located at about 42 degrees north latitude, we should expect to see evidence of ice and glacial features here, and that is exactly what both photos show.
» Read more

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Deployment process of Ingenuity begins

9:15 am

Ingenuity on the bottom of Perseverance
Click for full image.

Ingenuity vertical under Perseverance
Click for full image.

The photo to the right, cropped and reduced to post here, shows the Ingenuity helicopter attached to the base of the Perseverance rover, with its left end (the white box in the middle) now lowered. Previously the helicopter was stored horizontal against the rover’s base.

This photo was taken yesterday by Perseverance’s Watson camera, which provides images of the rover’s bottom and wheels.

The deployment process has only begun. They need to get that white box vertical and on the ground, then unfold the blades that are attached above it. I suspect as the base is dropped the two blades to the left will remain attached to Perseverance, thus partly unfolding them. I also suspect that full deployment of all four blades (the right two blades are what looks like a post with a bulbous end on the right of the base) will not occur until Ingenuity is fully detached and Perseverance has moved away. My error. I mistook the helicopter’s landing legs for its blades. Two of the legs (on the left) appear deployed, while two (on the right) remain in their stored position.

UPDATE: Ingenuity is now vertical, underneath Perseverance, as shown by the second image to the right.

These images are from yesterday, so these are actions that the rover and helicopter are doing autonomously. It appears from later images that the second set of legs began deploying next.

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Baffling ridges on Mars

1:01 pm

Baffling ridges on Mars
Click for full image.

Today’s cool image is one of my “what the heck?” photos. The picture to the right, cropped and reduced to post here and taken on September 3, 2020 by the high resolution camera on Mars Reconnaissance Orbiter (MRO), shows a strange dune field of many parallel long dunes, cross-cut by larger ridges.

Are the larger ridges dunes? Or are they some form of volcanic or tectonic ridge, which is also very typical of this region, called Tempe Terra and located in the transition zone between the southern cratered highlands and the northern lowland plains?

Or are they eskers, ridges frequently found in places that were once covered by glaciers? At 35 degrees north latitude, it would not be surprising to see glacial features here, but as far as I can tell, the full image has no obvious such features.
» Read more

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Ice-filled crater in Mars’ glacier country

2:06 pm

Crater filled with ice
Click for full image.

Cool image time! The photo to the right, cropped and reduced to post here and taken on January 7, 2021 by the high resolution camera on Mars Reconnaissance Orbiter (MRO), provides us a perfect example of the kind of glacial feature that scientists find routinely in the 30 to 60 degree mid-latitude bands on Mars. In this case the crater is in the northern reaches of a chaos region dubbed Nilosyrtis Mensae, the easternmost mensae region of what I dub glacier country on Mars.

When first identified scientists named this concentric crater fill, a purposely vague term that is only descriptive because they then did not know what it was made of, though they had their suspicions that it was buried glacial ice. Since then radar data has routinely confirmed that there is ice in such filled craters, making this particular glacial feature one of the most prevalent in those mid-latitude bands.

You can see a quite similar ice-filled crater, also in Nilosyrtis, in an earlier post from October 2020. While that earlier crater was on the southern edge of Nilosyrtis, today’s crater is about 300 miles almost due north, near the region’s northern fringe. In between are lots of similar glacial features, sometimes in craters, sometimes flowing off the slopes of mesas, and sometimes flow features in the open canyons between.

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Mars’ polar ice canyons are young and the source for mid-latitude ice

9:40 am

Mars' north pole icecap
Mars’ north polar ice cap.

Scientists have now proposed that the giant ice canyons seen at the edges of Mars’ polar ice caps are very young and are also the source of the water that sublimates away when the planet’s rotational tilt (its obliquity) is high, to fall as snow in the mid-latitudes where it forms the glaciers and ice sheets we now find there.

The image to the right, reduced to post here, shows the entire north pole ice cape on the left, with its spiral canyons. The two inserts on the bottom show for scale Hawaii’s Big Island and the Grand Canyon. From the release:

“Erosion formed a huge ice canyon system, and that erosion is a source of the long-known mid-latitude mantles on Mars,” said Rodriguez, lead author of “North polar trough formation due to in‑situ erosion as a source of young ice in mid‑latitudinal mantles on Mars” that appears in Nature Scientific Reports.

The troughs are arranged in a vast spiral pattern covering an area the size of Texas. We find that their growth lateral to katabatic wind (wind that carries high-density colder air from a higher elevation down a slope) directions produced widespread simple intersections, from which the highly complex spiral arrangement emerged, Rodriguez said. “The spiral pattern seen in the troughs is basically an erosional byproduct,” he said. “As the pits grow and intersect over a pre-existing dome-shaped polar cap, the spiral pattern emerges.

“It has long been proposed that sublimation of water ice from the north polar cap during high-obliquity cycles was an essential source of the planet’s mid-latitude icy plains. Our finding identifies the troughs as direct evidence of those sublimation phases,” Rodriguez said.

These spiral trough features formed very recently, in geologic terms: between a few million and 50,000 years ago, Rodriguez said.

This hypothesis, if true, is very important in understanding the long term geological history of Mars. The present theory is that when the obliquity rises to as high of 60 degrees, compared to today’s 25 degrees (similar to Earth’s), the mid-latitudes are colder than the poles, and the ice at the poles then migrates to the mid-latitudes. This paper gives us the place at the poles where the icecap shrinks as that ice sublimates away.

Knowing that these polar canyons are young and the source of the mid-latitude ice scientists can now begin to write the geological history of the polar ice caps themselves. They can also use this information to maybe determine whether the caps are presently in a steady state, as now believed, or growing or shrinking.

The youth of these canyons also suggests that any mid-latitude ice from them is also young, and thus more likely pure water unpoisoned by the toxic perchlorates found in many places on the Martian surface. It will thus be easier to obtain pure drinkable water from them.

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