jeudi 17 décembre 2020

Chang’e-5 landing and capsule recovery

 







CLEP - China Lunar Exploration Program logo.


Dec. 17, 2020

Chang’e-5 capsule recovery

The Chang’e-5 capsule reentered the Earth’s atmosphere and successfully landed under a parachute in Siziwang Banner, Inner Mongolia Autonomous Region, China, on 16 December 2020, at 17:59 UTC (17 December, 01:59 local time).

Chang’e-5 landing and capsule recovery

A fox was the first at the scene, but the rabbit Yutu was not onboard. The Chang’e-5 capsule was loaded onto a truck, then transported by helicopter and airplane to Beijing.

According to Lin Yangting (professor, Institute of Geology and Geophysics, Chinese Academy of Sciences), a joint team will be formed with European researchers to study the samples, part of the cooperation with the European Space Agency.

Related articles:

Chang’e-5 landed in Inner Mongolia
https://orbiterchspacenews.blogspot.com/2020/12/change-5-landed-in-inner-mongolia.html

Ready for Chang’e-5 landing
https://orbiterchspacenews.blogspot.com/2020/12/ready-for-change-5-landing.html

Chang’e-5 on the way to Earth
https://orbiterchspacenews.blogspot.com/2020/12/change-5-on-way-to-earth.html

Chang’e-5 completes first trans-Earth injection maneuver
https://orbiterchspacenews.blogspot.com/2020/12/change-5-completes-first-trans-earth.html

Chang’e-5 orbiter-sample return vehicle separates from ascender
https://orbiterchspacenews.blogspot.com/2020/12/change-5-orbiter-sample-return-vehicle.html

Chang’e-5 - Rendezvous and docking explained
https://orbiterchspacenews.blogspot.com/2020/12/change-5-rendezvous-and-docking.html

Chang’e-5 ascends to lunar orbit
https://orbiterchspacenews.blogspot.com/2020/12/change-5-ascends-to-lunar-orbit.html

Chang’e-5 collecting lunar samples
https://orbiterchspacenews.blogspot.com/2020/12/change-5-collecting-lunar-samples.html

Chang’e-5 lands on the Moon
https://orbiterchspacenews.blogspot.com/2020/12/change-5-lands-on-moon.html

Chang’e-5 ready for Moon landing
https://orbiterchspacenews.blogspot.com/2020/11/change-5-ready-for-moon-landing.html

Chang’e-5 enters lunar orbit
https://orbiterchspacenews.blogspot.com/2020/11/change-5-enters-lunar-orbit.html

Chang’e-5 completes first orbital correction
https://orbiterchspacenews.blogspot.com/2020/11/change-5-completes-first-orbital.html

CASC - Long March-5 Y5 launches Chang’e-5 lunar mission
https://orbiterchspacenews.blogspot.com/2020/11/casc-long-march-5-y5-launches-change-5.html

ESA tracks Chang'e-5 Moon mission
https://orbiterchspacenews.blogspot.com/2020/11/esa-tracks-change-5-moon-mission.html

For more information about China Aerospace Science and Technology Corporation (CASC), visit: http://english.spacechina.com/n16421/index.html

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

The surprises of the Standard Model at high energies

 







CERN - European Organization for Nuclear Research logo.


Dec. 17, 2020

In the seventh part of the LHC Physics at Ten series, we look at the surprising phenomena of the Standard Model at high energies

"Robust” is what scientists working on the Large Hadron Collider (LHC) like to use to describe the Standard Model. By stubbornly probing it for weaknesses over the past 10 years, they have run up against the extreme solidity of this theory, which describes particles and forces. However, particle physicists are well aware that this model, finalised in the 1970s, has a few shortcomings. They are therefore searching for a wider theory that could resolve certain mysteries, and are banking on the LHC to help them find it. But apart from the triumphant discovery of the Higgs boson, no other new fundamental particle has been discovered, nor any extraordinary phenomenon that might lead to a more comprehensive theory.

Large Hadron Collider (LHC). Animation Credit: CERN

Has all this deterred them from their quest? “Quite the opposite,” smiles Nadjieh Jafari, co-leader of the top-quark group at the CMS experiment. “There are many different territories for us to explore with the LHC: it’s an exciting period.” By venturing to the highest energies ever reached, physicists are observing many phenomena that were previously out of their reach.

“We are measuring the behaviour of nature at new energies,” says Jonathan Butterworth, a physicist with the ATLAS experiment. “Even though they fit with the Standard Model, these phenomena are totally new to us.”

New energies bring new phenomena

The physicists at ATLAS are interested, for example, in the high-energy transverse jets of quarks and gluons. These jets can contain massive particles such as the W and Z bosons, the messenger particles of the weak force. “These new observations open up fields of research on the structure of such jets, to help us understand the strong interaction, as well as the electroweak interaction when a W or Z boson is emitted,” says Butterworth. The image above shows an ATLAS experiment event with two such jets (yellow and green cones).

The experiments are therefore examining every square centimetre of this new territory, looking for processes that have been predicted but are either extremely rare, have never been observed before, or even better, are completely unexpected. These experiments include ATLAS and CMS, which observe the fusion and diffusion of electroweak bosons – very rare interactions. These events produce W and Z bosons, which either fuse together to produce another particle (fusion) or bounce away from each other (diffusion). “It’s as if the LHC had become a collider of weak bosons; these phenomena are completely new at these energies,” says Paolo Azzurri, co-leader of the Standard Model group at CMS.


Images above: On the left, a CMS event display of a candidate event in which two W bosons and one Z boson are produced. On the right, an ATLAS event display of a candidate event in which two Z bosons are produced. (Image: CMS and ATLAS, CERN).

Another observation in this region, which is around 50 times rarer than the production of the Higgs boson, is the simultaneous production of three weak bosons. This phenomenon is seen only once in approximately every 100 billion proton collisions. These interactions also provide a new tool with which to probe the Standard Model and the weak interaction carried by the W and Z bosons. “The programme of boson fusion and diffusion started recently,” says Andrew Pilkington, a physicist with the ATLAS experiment. “There is still a long way to go before we can move from observation to the precision measurements that could allow us to detect deviations.”

The promise of virtual particles

Physicists measure the frequency of these phenomena (their cross section) as precisely as possible and compare it with theoretical predictions. Any difference could indicate the presence of new particles. If unknown particles exist, they may be too massive to be produced at the LHC, but their quantum behaviour could help spot them.“In quantum field theory, anything that isn’t forbidden can happen,” explains Claude Duhr, a theoretical physicist at CERN. “Particles that are too massive to be produced in reality may appear and disappear fleetingly during an interaction.” These particles are known as virtual particles: they are involved in the interaction, but they are not directly detected. “We can deduce their presence because they have an impact on the interaction. For example, we could observe an excess of events during an interaction, which would indicate the presence of virtual particles,” continues Duhr. This is why it is necessary to measure interactions very precisely, in order to be able to compare the results with the theoretical predictions.

However, one big difficulty is obtaining precise theoretical predictions. Due to the virtual particles, there are not just one but many ways in which the particles can be produced during a proton collision. Physicists have to take into account not only the direct processes (leading order or LO), in which these particles are directly produced without any contribution from virtual particles, but also the processes that result from the appearance of a virtual particle (next-to-leading order or NLO) or even two virtual particles (next-to-next-to-leading order or NNLO) and so on.

These processes with the appearance of virtual particles occur more frequently when the strong interaction is involved (which is the case for proton collisions) and when the energy level is high. It is crucial to take them into account for certain interactions, such as the production of the Higgs boson. However, these “perturbative” theoretical calculations are very complex and have required physicists to develop new mathematical tools, spurred on by the results from the LHC experiments. “It took four people four years to calculate the production of the Higgs boson at the next-to-next-to-leading order NNLO,” explains Duhr, a specialist in this field. And physicists are studying numerous interactions at the LHC, which pushes theorists to carry out many perturbative calculations to allow a comparison with the theory.

To make things even more challenging, the theoretical predictions also rely on solid knowledge of the proton. Paradoxically, the proton, which makes up all the matter around us, is a complex system and its structure is poorly understood. Its three quarks are bound by the strong force, which acts through the exchange of gluons, the messenger particles of the strong interaction. Determining the distribution of a given proton energy among the components of the proton (which we also refer to as partons) is anything but simple. This information is important to understand the initial conditions or, in other words, the energy available during the collision. “The huge amounts of data from the LHC have allowed us to considerably improve our understanding of the structure of the proton,” says Giorgio Passaleva, a physicist with the LHCb experiment.

The top quark: a massive effect


Image above: Event recorded by the CMS experiment in 2016 in which four top quarks were produced simultaneously (Image: CMS/CERN).

Among the many studies of the Standard Model, those relating to the top quark are particularly special. The top quark is the heaviest of the quarks and is almost 90 000 heavier than the lightest, the up quark. It has a very strong coupling with the Higgs boson, which is to be expected since the mechanism associated with this boson that gives elementary particles their mass. As the top quark is also sensitive to the strong, weak and electromagnetic forces, it can be produced by a myriad of processes. It is therefore an ideal candidate for exploring the new energy territories made accessible by the LHC. Florencia Canelli, co-leader of the top-quark physics group at the CMS experiment, started working on the topic at Fermilab in the US in 1998, three years after the laboratory discovered the quark. Pioneering studies were carried out at the Tevatron to define the top quark’s characteristics but, for the past 10 years, the LHC has provided an excellent observation ground for this particle. In the space of just a few years, ATLAS and CMS have been able to measure the mass of the top quark with excellent precision.

“With the LHC, we have access to unexplored regions and huge amounts of data, which allow us to gain a more complete and precise understanding of the top quark. These measurements also allow us to constrain new physics processes,” explains Florencia Canelli, CMS physicist.


Image above: Event recorded in 2018 by the ATLAS experiment in which four top quarks are produced. (Image: ATLAS/CERN).

The high energies at the LHC also provide an opportunity to study the production of top quarks with massive particles such as the W and Z bosons. “Or the simultaneous production of four top quarks, a quite extraordinary phenomenon,” confirms her colleague Nadjieh Jafari, who has been working on the subject since 2008 and is now co-leader of the CMS top-quark analysis group.

The study of the top quark is one of the main focuses of the search for physics beyond the Standard Model. It is thought that unknown particles with a higher mass could decay into top quarks. “The top quark opens a door to theories beyond the Standard Model. Many predict new particles would decay into top quarks or into the same final states as those of the top quark,” confirms Francesco Spano, co-leader of the ATLAS top-quark analysis group.

The study of the interactions involving this special particle is far from complete. Wolfgang Wagner, a physicist with the ATLAS experiment, displays a table indicating the different processes producing the top quark at the LHC and the analyses carried out for each of them. 19 of the 48 boxes in his table are marked with a cross, indicating that the process in question has been studied. “Ten years ago, we were just starting the study of the production of top-antitop pairs, the most accessible of the processes. Today, we have exceeded the precision of the theory for this process, but we still have many other processes to examine,” he explains.

Strange assemblies


Image above: Illustration of the possible layout of quarks in a pentaquark particle, such as those discovered at LHCb. (Image: Daniel Dominguez/CERN).

In its exploration of these new energy territories, LHCb has unearthed exotic assemblies of quarks in which four or even five quarks are bound by the strong interaction. According to the model of hadrons, there are two categories of composite particles: mesons, composed of pairs containing a quark and an antiquark, and baryons, such as protons, containing three quarks. In the quark model proposed in 1964, Murray Gell-Mann and George Zweig also predicted the possible existence of exotic hadrons such as tetraquarks and pentaquarks.

In 2010, LHCb spotted its first tetraquark, followed by several others over the course of the last 10 years. In 2015, the experiment created a stir by announcing the first discovery of a pentaquark. In 2019, a second pentaquark was identified. “These exotic systems are so extreme and strange that they have aroused the interest of theoretical physicists,” explains Giovanni Passaleva, a physicist and former LHCb spokesperson. In fact, the appearance of these exotic hadrons has inspired new research in order to understand their internal mechanisms.

“The study of these exotic assemblies is another tool for testing the hadron model and quantum chromodynamics, the theory of the strong interaction,” adds Tatsuya Nakada, the first spokesperson of LHCb.The experimental data on exotic hadrons will allow physicists to improve their understanding of quantum chromodynamics at low energies, which describes the bound states of quarks.

LHCb physicists are pursuing their examination of this small corner of the Standard Model, just like all the other thousands of LHC scientists studying the new areas opened up by the LHC. Even though the number of events produced by the LHC is already phenomenal, large quantities of data are still required to understand these new phenomena in detail. The Standard Model is robust, so scientists need patience and precision to find its limits.

“We explore nature by getting close to the conditions at the very beginning of time, on the smallest scales ever achieved, and we look for deviations from our expectations. It’s in these minuscule regions of space and time that we will be able to detect the limits of the Standard Model,” concludes Francesco Spano, ATLAS physicist.

Note:

CERN, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works. At CERN, the world’s largest and most complex scientific instruments are used to study the basic constituents of matter — the fundamental particles. By studying what happens when these particles collide, physicists learn about the laws of Nature.

The instruments used at CERN are particle accelerators and detectors. Accelerators boost beams of particles to high energies before they are made to collide with each other or with stationary targets. Detectors observe and record the results of these collisions.

Founded in 1954, the CERN Laboratory sits astride the Franco–Swiss border near Geneva. It was one of Europe’s first joint ventures and now has 23 Member States.

Related links:

Large Hadron Collider (LHC): https://home.cern/science/accelerators/large-hadron-collider

CMS experiment: https://home.cern/science/experiments/cms

Standard Model: https://home.cern/science/physics/standard-model

For more information about European Organization for Nuclear Research (CERN), Visit: https://home.cern/

Images (mentioned), Animation (mentioned), Text, Credits: CERN/By Corinne Pralavorio.

Best regards, Orbiter.ch

On the Hunt for a Missing Giant Black Hole

 







NASA - Chandra X-ray Observatory patch.


Dec. 17, 2020

The mystery surrounding the whereabouts of a supermassive black hole has deepened.

Despite searching with NASA's Chandra X-ray Observatory and Hubble Space Telescope, astronomers have no evidence that a distant black hole estimated to weigh between 3 billion and 100 billion times the mass of the Sun is anywhere to be found.

Supermassive black hole seen in X-ray

This missing black hole should be in the enormous galaxy in the center of the galaxy cluster Abell 2261, which is located about 2.7 billion light years from Earth. This composite image of Abell 2261 contains optical data from Hubble and the Subaru Telescope showing galaxies in the cluster and in the background, and Chandra X-ray data showing hot gas (colored pink) pervading the cluster. The middle of the image shows the large elliptical galaxy in the center of the cluster.

Nearly every large galaxy in the Universe contains a supermassive black hole in their center, with a mass that is millions or billions of times that of the Sun. Since the mass of a central black hole usually tracks with the mass of the galaxy itself, astronomers expect the galaxy in the center of Abell 2261 to contain a supermassive black hole that rivals the heft of some of the largest known black holes in the Universe.

Using Chandra data obtained in 1999 and 2004 astronomers had already searched the center of Abell 2261's large central galaxy for signs of a supermassive black hole. They looked for material that has been superheated as it fell towards the black hole and produced X-rays, but did not detect such a source.

Now, with new, longer Chandra observations obtained in 2018, a team led by Kayhan Gultekin from the University of Michigan in Ann Arbor conducted a deeper search for the black hole in the center of the galaxy. They also considered an alternative explanation, in which the black hole was ejected from the host galaxy's center. This violent event may have resulted from two galaxies merging to form the observed galaxy, accompanied by the central black hole in each galaxy merging to form one enormous black hole.

When black holes merge, they produce ripples in spacetime called gravitational waves. If the huge amount of gravitational waves generated by such an event were stronger in one direction than another, the theory predicts that the new, even more massive black hole would have been sent careening away from the center of the galaxy in the opposite direction. This is called a recoiling black hole.

Astronomers have not found definitive evidence for recoiling black holes and it is not known whether supermassive black holes even get close enough to each other to produce gravitational waves and merge; so far, astronomers have only verified the mergers of much smaller black holes. The detection of recoiling supermassive black holes would embolden scientists using and developing observatories to look for gravitational waves from merging supermassive black holes.

The galaxy at the center of Abell 2261 is an excellent cluster to search for a recoiling black hole because there are two indirect signs that a merger between two massive black holes might have taken place. First, data from the Hubble and Subaru optical observations reveal a galactic core — the central region where the number of stars in the galaxy in a given patch of the galaxy is at or close to the maximum value — that is much larger than expected for a galaxy of its size. The second sign is that the densest concentration of stars in the galaxy is over 2,000 light years away from the center of the galaxy, which is strikingly distant.

These features were first identified by Marc Postman from Space Telescope Science Institute (STScI) and collaborators in their earlier Hubble and Subaru images, and led them to suggest the idea of a merged black hole in Abell 2261. During a merger, the supermassive black hole in each galaxy sinks toward the center of the newly coalesced galaxy. If they become bound to each other by gravity and their orbit begins to shrink, the black holes are expected to interact with surrounding stars and eject them from the center of the galaxy. This would explain Abell 2261's large core. The off-center concentration of stars may also have been caused by a violent event such as the merger of two supermassive black holes and subsequent recoil of single, larger black hole that results.

Even though there are clues that a black hole merger took place, neither Chandra nor Hubble data showed evidence for the black hole itself. Gultekin and most of his co-authors, led by Sarah Burke-Spolaor from West Virginia University, had previously used Hubble to look for a clump of stars that might have been carried off by a recoiling black hole. They studied three clumps near the center of the galaxy, and examined whether the motions of stars in these clumps are high enough to suggest they contain a ten billion solar mass black hole. No clear evidence for a black hole was found in two of the clumps and the stars in the other one were too faint to produce useful conclusions.

They also previously studied observations of Abell 2261 with the NSF's Karl G. Jansky Very Large Array. Radio emission detected near the center of the galaxy showed evidence that supermassive black hole activity had occurred there 50 million years ago, but does not indicate that the center of the galaxy currently contains such a black hole.

They then turned to Chandra to look for material that had been superheated and produced X-rays as it fell towards the black hole. While the Chandra data did reveal that the densest hot gas was not in the center of the galaxy, they did not reveal any possible X-ray signatures of a growing supermassive black hole — no X-ray source was found in the center of the cluster, or in any of the clumps of stars, or at the site of the radio emission.


 Chandra X-ray Observatory

The authors concluded that either there is no black hole at any of these locations, or that it is pulling material in too slowly to produce a detectable X-ray signal.

The mystery of this gigantic black hole's location therefore continues. Although the search was unsuccessful, hope remains for astronomers looking for this supermassive black hole in the future. Once launched, the James Webb Space Telescope may be able to reveal the presence of a supermassive black hole in the center of the galaxy or one of the clumps of stars. If Webb is unable to find the black hole, then the best explanation is that the black hole has recoiled well out of the center of the galaxy.

A paper describing these results has been accepted for publication in a journal of the American Astronomical Society, and is also available online at https://arxiv.org/abs/2010.13980. Gultekin's co-authors are Sarah Burke-Spolaor; Tod R. Lauer (National Optical Infrared Astronomy Research Laboratory, Tucson, Arizona); T. Joseph W. Lazio and Leonidas A. Moustakas (Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California); and Patrick Ogle and Marc Postman (Space Telescope Science Institute, Baltimore, Maryland).

NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts.

Read more from NASA's Chandra X-ray Observatory: https://chandra.harvard.edu/photo/2020/a2261/

For more Chandra images, multimedia and related materials, visit: http://www.nasa.gov/chandra

Image, Animation, Text, Credits: X-ray: NASA/CXC/Univ of Michigan/K. Gültekin; Optical: NASA/STScI and NAOJ/Subaru; Infrared: NSF/NOAO/KPNO/NASA/Lee Mohon.

Greetings, Orbiter.ch

Solar Orbiter prepares for festive Venus flyby

 







ESA & NASA - Solar Orbiter Mission patch.


Dec. 17, 2020

Solar Orbiter is getting ready for the first of many gravity assist flybys of Venus on 27 December, to start bringing it closer to the Sun and tilting its orbit in order to observe our star from different perspectives.

Solar Orbiter flyby of Venus

Just as the majority of us will remain safely at home under various COVID-19 pandemic lockdown measures during what is traditionally a holiday period, the flyby – a routine event in the world of flying spacecraft – will also be monitored by the spacecraft operations managers remotely as well.

Closest approach will take place at 12:39 UTC (13:39 CET) on 27 December, and will see the spacecraft fly some 7 500 km from the Venus cloud tops.  Later flybys, from 2025, will see much closer encounters of just a few hundred kilometres.

Solar Orbiter Venus flyby

During the upcoming flyby several in-situ science instruments – MAG, RPW and some sensors of EPD – will be switched on to record the magnetic, plasma and particle environment around the spacecraft as it encounters Venus. (It is not possible to take images of Venus during the flyby because the spacecraft must remain facing the Sun.)

In order to properly line up for the flyby, specialists from ESA's ground stations and flight dynamics teams conducted a so-called ‘Delta-DOR’ campaign, using an advanced technique – Delta-Differential One-Way Ranging – to precisely determine the spacecraft's position in space, and its trajectory.

Ultra-precise navigation

In Delta-DOR, a set of widely separated ground stations on Earth are used to receive the spacecraft's radio signals, giving a first result for its location. Then, this result is compared to locations of known stellar radio sources previously mapped by other missions, resulting in a corrected and ultra-precise final plot. The Delta-DOR technique allows operators to determine where a spacecraft is to within a few hundred metres, even at a distance of 100 million km.

Solar Orbiter's journey around the Sun

Today, 17 December, Solar Orbiter is 235 million kilometres from Earth, and about 10.5 million from Venus. It takes about 13 minutes for signals to travel to (or from) the spacecraft.

Solar Orbiter’s path around the Sun has been chosen to be ‘in resonance’ with Venus, which means that it will return to the planet’s vicinity every few orbits and can again use the planet’s gravity to alter or tilt its orbit. The next encounter will be in August 2021, which is also within a few days of BepiColombo’s next Venus gravity assist. Initially Solar Orbiter will be confined to the same plane as the planets, but each encounter of Venus will increase its orbital inclination. By 2025 it will make its first solar pass at 17º inclination, increasing to 33º by the end of the decade, bringing even more of the polar regions into direct view. This will result in the spacecraft being able to take the first ever images of the Sun’s polar regions, crucial for understanding how the Sun ‘works’, for investigating the Sun-Earth connection and how we can better predict periods of stormy space weather.

Solar Orbiter is a space mission of international collaboration between ESA and NASA.

Related link:

Solar Orbiter: https://www.esa.int/Science_Exploration/Space_Science/Solar_Orbiter

Images, Videos, Text, Credits: ESA/ATG medialab.

Greetings, Orbiter.ch

Dreaming of a red Christmas: Festive features spotted near Mars’ south pole

 







ESA - Mars Express Mission patch.


Dec. 17, 2020

As the holiday season swiftly approaches, even our planetary neighbours are getting into the spirit – as shown by this perfect pair of festive silhouettes spotted by ESA’s Mars Express.

Festive silhouettes near Mars’ south pole

The defined wings of an angelic figure, complete with halo, can be seen sweeping up and off the top of the frame in this image from Mars Express’ High Resolution Stereo Camera, while a large heart sits just right of centre. These shapes appear to jump out of the light tan — or, in the spirit of the season, eggnog-coloured! — surface of Mars; their dark colour is a result of the composition of the constituent dune fields, which largely comprise sands rich in dark, rock-forming minerals that are also found on Earth (namely pyroxene and olivine).

In context: A festive scene near Mars’ south pole

This ethereal scene is found in the south polar region of Mars, with the pole itself located directly out of frame to the right (south). The south pole is typically covered in a 1.5 km-thick ice cap measuring around 400 km across and with a volume of 1.6 million cubic kilometres, just over 12% of which is water ice.  The rest of the cap is largely composed of ‘dry ice’ (solid carbon dioxide), which freezes from the atmosphere during winter and then sublimates (turns from a solid to a gas) in the summer.

As Mars’ southern hemisphere is currently experiencing summer, this image shows the planet’s southern polar ice stores at their lowest annual levels.

Perspective view: An angel and heart on Mars

The ‘angel’ and ‘heart’ are both composed of various interesting features. Firstly, the angel’s hand, seen as if reaching to the left, is thought to be a large sublimation pit, a type of feature that forms as ice turns to gas and leaves empty pockets and depressions in the planetary surface (a process that often occurs as the seasons change). Sublimation pits have been seen on other planets in the Solar System, such as Pluto, and can also be seen scattered across the terrain to the right.

Topographic view of an angel and heart on Mars

Moving on to one of the angel’s most distinctive features, its halo, reveals yet more intriguing processes at play. The ‘head’ and halo are formed of an impact crater, created as a body from space flew inwards to collide with Mars’ crust. As this impactor hit it dug down into the surface, revealing the numerous layered deposits that make up the southern polar region. These subsurface layers can be glimpsed in other areas where the surface has been disturbed – areas that are clearly identifiable in the associated topographic view due to their notably low elevation – and hint at the long, complex, interesting history of this part of Mars.

Perspective view: A heart on Mars

Finally comes the heart, which is underscored by a steep escarpment – a line of cliffs or steep slopes created by erosive processes – and separated from the dark expanse of dunes below. The origin of this dark material, which is found all over Mars, remains unclear, but scientists posit that it once existed deeper below the surface in layers of material formed by ancient volcanic activity. Although this material was initially buried, it has since been brought to the surface by ongoing impacts and erosion, and then distributed more widely across the planet by martian winds.

Mars Express

This landscape also shows signs of dust devils in the dark, scratched, cross-hatched pattern to the left of the frame. Dust devils are common on Mars, and form as dust is whipped up from the Sun-warmed surface by wind. Here, dust devils have lifted surface material and carried it away, leaving dark marks in their wake.

A festive scene near Mars’ south pole – in 3D

The south pole of Mars is a fascinating region – and a watery one. Just a few months ago, Mars Express found signs of three new ponds of salty liquid water thought to be buried below the ice here, adding to the discovery of a large underground reservoir in 2018. Although the Red Planet appears dry and lifeless today, it was once far warmer and wetter, much like the early Earth. While the surface may no longer be hospitable to water, its subsurface may remain a friendly environment for ancient lake systems that, excitingly, may hold evidence of life on Mars.

As many gear up for a safe and restful Christmas period, Mars Express will not rest on its laurels; the spacecraft will continue to observe and image our planetary neighbour in detail, as it has done since it entered orbit around Mars in December 2003. The mission has revealed an astonishing amount about Mars in this time, helping us to better understand the planet’s water, geology, chemistry, atmosphere, moons, history, context in the Solar System, and much more.

Related links:

Mars Express’ High Resolution Stereo Camera: https://www.esa.int/ESA_Multimedia/Images/2004/01/The_High_Resolution_Stereo_Camera_HRSC

Mars Express: https://www.esa.int/Science_Exploration/Space_Science/Mars_Express

Images, Text, Credits: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO/NASA MGS MOLA Science Team.

Best regards, Orbiter.ch

mercredi 16 décembre 2020

Space Biology on Station Seeks to Improve Human Health

 






ISS - Expedition 64 Mission patch.


Dec. 16, 2020

Space biology was the dominant research theme aboard the International Space Station today. The Expedition 64 crew explored heart cells, muscles and more to understand how microgravity impacts the human body.

The Cardinal Heart study has been under way all week with the crew observing engineered heart tissue samples through a microscope in Japan’s Kibo laboratory module. The samples are being processed inside the Life Sciences Glovebox to help researchers understand and treat abnormal heart cells and tissues that can lead to disease both on Earth and in space.


Image above: Expedition 64 Flight Engineer Soichi Noguchi gives a “thumbs up” inside the seven-windowed cupola, the International Space Station’s “window to the world.” Image Credit: NASA.

The lack of gravity aboard the space station means astronauts exert less energy when moving around the orbiting lab resulting in muscle atrophy. Daily exercise offsets this loss and keeps crew members healthy and strong during long term missions and prepares them for the return to Earth after months of living in space.

The Myotones study taking place today seeks to understand the biochemical properties of muscles exposed to weightlessness. Analysis of ultrasound scans and blood samples taken from crew members could give scientists insights into muscle conditions caused by lack of movement and aging.

View from ISS. Animation Credit: ISS HD Live Now

Organ transplants are critical on Earth especially with demand exceeding supply. Doctors are exploring generating cell growth in three dimensions and creating artificial organs in space since Earth’s gravity limits this growth. The new Space Organogenesis study ongoing this month uses the space station to enable 3D cell growth to promote regenerative technology and someday support patients on Earth who need transplants.

Related links:

The Expedition 64: https://www.nasa.gov/mission_pages/station/expeditions/expedition64/index.html

Cardinal Heart: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8218

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

Life Sciences Glovebox: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Facility.html?#id=7676

Myotones: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=7573

Space Organogenesis: https://www.nasa.gov/mission_pages/station/research/experiments/explorer/Investigation.html?#id=8116

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

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

Best regards, Orbiter.ch

Chang’e-5 landed in Inner Mongolia

 







CLEP - China Lunar Exploration Program logo.


Dec. 16, 2020

Chang’e-5 landed in Inner Mongolia (infrared image)

The Chang’e-5 sample return vehicle successfully landed in Siziwang Banner, Inner Mongolia Autonomous Region, China, on 16 December 2020, at 17:59 UTC (17 December, 01:59 local time).

Chang’e-5 landed in Inner Mongolia

Chang’e-5 is China’s first lunar mission to collect soil samples from the Moon and returns them to Earth to be studied. Chang’e-5 collected samples near Mons Rümker, in the northern region of Oceanus Procellarum, a younger volcanic complex.

According to Lin Yangting (professor, Institute of Geology and Geophysics, Chinese Academy of Sciences), a joint team will be formed with European researchers to study the samples, part of the cooperation with the European Space Agency.

Related articles:

Ready for Chang’e-5 landing
https://orbiterchspacenews.blogspot.com/2020/12/ready-for-change-5-landing.html

Chang’e-5 on the way to Earth
https://orbiterchspacenews.blogspot.com/2020/12/change-5-on-way-to-earth.html

Chang’e-5 completes first trans-Earth injection maneuver
https://orbiterchspacenews.blogspot.com/2020/12/change-5-completes-first-trans-earth.html

Chang’e-5 orbiter-sample return vehicle separates from ascender
https://orbiterchspacenews.blogspot.com/2020/12/change-5-orbiter-sample-return-vehicle.html

Chang’e-5 - Rendezvous and docking explained
https://orbiterchspacenews.blogspot.com/2020/12/change-5-rendezvous-and-docking.html

Chang’e-5 ascends to lunar orbit
https://orbiterchspacenews.blogspot.com/2020/12/change-5-ascends-to-lunar-orbit.html

Chang’e-5 collecting lunar samples
https://orbiterchspacenews.blogspot.com/2020/12/change-5-collecting-lunar-samples.html

Chang’e-5 lands on the Moon
https://orbiterchspacenews.blogspot.com/2020/12/change-5-lands-on-moon.html

Chang’e-5 ready for Moon landing
https://orbiterchspacenews.blogspot.com/2020/11/change-5-ready-for-moon-landing.html

Chang’e-5 enters lunar orbit
https://orbiterchspacenews.blogspot.com/2020/11/change-5-enters-lunar-orbit.html

Chang’e-5 completes first orbital correction
https://orbiterchspacenews.blogspot.com/2020/11/change-5-completes-first-orbital.html

CASC - Long March-5 Y5 launches Chang’e-5 lunar mission
https://orbiterchspacenews.blogspot.com/2020/11/casc-long-march-5-y5-launches-change-5.html

ESA tracks Chang'e-5 Moon mission
https://orbiterchspacenews.blogspot.com/2020/11/esa-tracks-change-5-moon-mission.html

For more information about China Aerospace Science and Technology Corporation (CASC), visit: http://english.spacechina.com/n16421/index.html

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