Ancient Martian Rivers Revealed In Satellite Images

Ancient Martian rivers revealed in satellite images

ESA's Mars Express orbiter has captured some stunning images of dry riverbeds on Mars
ESA’s Mars Express orbiter has captured some stunning images of dry riverbeds on Mars

The Red Planet is notoriously dry and dusty, but its scarred surface shows that that wasn’t always the case. A new set of photos from the European Space Agency’s Mars Express orbiter demonstrates some pretty clear evidence of an ancient river network that once wound across the Martian landscape.

While modern day Mars is drier than any Earthly desert, it’s believed that roughly 4 billion years ago the Red Planet was much bluer, with a northern ocean bigger than the Atlantic. Over the years, the many eyes on Mars have spotted signs of ancient shorelineslakesflood plainsrivers and glaciers. That makes the newest European Space Agency (ESA) shots not particularly surprising, but no less beautiful.

The ancient riverbeds are clear in this image snapped by the Mars Express orbiter

These images were snapped on the southern highlands of Mars, a region pockmarked with craters and rich with evidence of old waterways. In this case, that takes the form of a branching network of valleys, snaking across the landscape to form shapes that are instantly recognizable as the handiwork of water.

Judging by the topography, water seems to have flowed downhill from north to south, which is right to left in these shots. The valleys left behind are up to 2 km wide and as deep as 200 m in places. That’s particularly clear in the topographic view, where red is the highest ground, and it turns yellow, then green and blue the lower you go.

This topographic image shows how the water would have flowed downhill from north to south (right...

The structures resemble drainage systems seen here on Earth, suggesting they were formed as excess water ran off from stronger rivers and made its own way downhill.

While the bulk of that water has likely been lost to space, there are indications that some of it is still locked away underground, in the form of ice sheets or even liquid lakes. These stashes could be vital resources for eventual human colonists.

Source: ESA

Now You Can Get Daily Weather Reports From Mars

If you’ve ever wondered what the weather is on Mars, wonder no more. Today, NASA published an online tool that will allow the public to get daily Martian weather reports based on data gathered by the space agency’s unmanned InSight lander and includes a 24-hr breakdown of the Red Planet’s temperature, wind, and air pressure.

Getting weather reports from Mars isn’t anything new. Astronomers have been trying to puzzle out Martian meteorology for centuries using Earthbound telescopes and on-the-spot measurements have been available since the Viking landers successfully touched down in 1976.

However, the InSight mission has upped the game because its objective of studying the interior structure and dynamics of the planet requires keeping things as quiet as possible in the vicinity of the instruments to cut out interference. That isn’t possible with a small robotic lander, so mission scientists compensate by measuring vibrations caused by wind and pressure changes as well as temperature fluctuations, then cancelling them out mathematically.

Artist's concept shows NASA's InSight lander with its instruments deployed on the Martian surface

It’s for this reason that InSight is equipped with the Auxiliary Payload Subsystem (APSS) instrument package that monitors the weather 24 hours a day – or 24 hours, 39 minutes, since we’re talking about Mars. This helps keep the Seismic Experiment for Interior Structure (SEIS) accurate by not only looking at standard weather parameters, but also the local magnetic field thanks to a UCLA-made magnetometer found under the edge of the lander’s deck.

Air temperature and wind sensors known as the Temperature and Wind for InSight (TWINS) sit on booms located on the lander’s deck. Built by Spain’s Centro de Astrobiología, TWINS detects strong winds that could mess with seismic monitoring and works in conjunction with the lander’s cameras to help better understand how the wind picks up the dust on the Martian surface.

The online Mars weather tool was made by the Jet Propulsion Laboratory in Pasadena, California, Cornell University, and Centro de Astrobiología in Madrid. Oh, and if you’re interested, the weather on February 17 was a high of 2⁰ F (-17º C), a low of -138º F (-95º C), and SW winds of 37.8 mph (60.8).

The daily Martian weather reports are available here.

Source: NASA

What Are The Mysterious “Slope Streaks” On Mars

Ron Clatworthy

5:31 AM (4 hours ago)

to me

What Are these Mysterious “Slope Streaks” on Mars?

Since they were first observed in the 1970s by the Viking missions, the slope streaks that periodically appear along slopes on Mars have continued to intrigue scientists. After years of study, scientists still aren’t sure exactly what causes them. While some believe that “wet” mechanisms are the culprit, others think they are the result of “dry” mechanisms.

Luckily, improvements in high-resolution sensors and imaging capabilities — as well as improved understanding of Mars’ seasonal cycles — is bringing us closer to an answer. Using a terrestrial analog from Bolivia, a research team from Sweden recently conducted a studythat explored the mechanisms for streak formation and suggests that wet mechanisms appear to account for more, which could have serious implications for future missions to Mars.

The study, titled “Are Slope Streaks Indicative of Global?Scale Aqueous Processes on Contemporary Mars?”, recently appeared in the Reviews of Geophysics, a publication maintained by the American Geological Union (AGU). The study was conducted by Anshuman Bhardwaj and his colleagues, all of whom hail from the Luleå University of Technology in Sweden.

As the team stated in a recent interview with the AGU’s Earth and Space Science News:

“What we know from observations is the following: Slope streaks range from about a few meters to several kilometers long. They usually have a starting point upslope with gradual widening towards the downslope termini, thus indicating the possible involvement of some flow or mass movement. They are capable of following very gentle slopes and are reportedly able to climb even a few meters of obstacles in their flow paths. Slope streaks can appear anytime of the year in the equatorial and subequatorial regions of Mars. They appear to be singular events formed within a short temporal span, and their recurrence, or lengthening, is extremely rarely observed. They gradually fade over decadal timescales.”

Despite the progress that has been made in studying these features, the scientific community remains divided into two camps when it comes to what causes Martian slope streaks. Those who belong to the “wet” mechanism school of thought believe that liquid water could be responsible for their creation, possibly as a result of groundwater springs, melting surface ice, or the formation of brines (salt solutions).

In contrast, those who fall into the “dry” mechanism school theorize that dust avalanches are responsible. These, in turn, could be caused by air fall deposits, subsurface melting, or localized disturbances — ranging by rockfalls, meteorite impacts, or tectonic activity (“Marsquakes”). Both of these explanations have limitations when it comes to explaining observed slope streaks.

For example, the main issue with the wet mechanism explanation is that observations have shown a lack of consistency when it comes to seasonal change. If liquid water or brines were the mechanism, then such slopes should only appear in areas that are experiencing warmer seasonal temperatures, which has not always been the case.

What’s more, slope streaks have been found to climb over obstacles in many instances, which is not consistent with liquid-driven displacement. Similarly, the dry mechanism explanation also suffers from a number of inconsistencies and challenges when considered on its own.

For starters, if slope streaks were caused by the displacement of dry mass, scientists would have observed disturbances alongside them, not to mention a buildup of debris at their lowest point downslope. In the majority of cases, neither of these have been observed. At the same time, dry mechanisms cannot explain why some streak formations extend for kilometers.

To shed further light on this, the team investigated a “wet analog” site in Salar de Uyuni, an Andean region in southwest Bolivia. This region, which is the largest salt flat in the world, experiences similar atmospheric and surface conditions as the equatorial region of Mars. This results in seasonal brine flows where chloride and sulphate salts become liquefied and create slope streaks.

After conducting drone-based observations of the region, the team determined that these streaks are a sufficient analog for a wet mechanism on Mars. They also recommend further studies, which could provide important clues about Martian brines and other surface features that have been linked to the transient occurrence of liquid water on Mars. As they conclude:

“While available remote sensing data has vastly improved, as well as our knowledge of Martian mineralogy, climate, and atmosphere, we still need further investigations to advance our understanding. In this regard, targeting slope streak regions during future robotic or manned Mars missions would be advantageous.”

Essentially, salt water or liquid flows could explain many of Mars’ slope streaks, but certain inconsistencies demand further research. Over time, we may learn that other mechanisms are involved, which could range from subsurface features to specific seasonal changes.

The subject of what causes these streaks and other transient surface features is important for many reasons, not the least of which has to do with planetary protection. In Sept. 2016, the Curiosity roverencountered dark streaks while driving along the sloping terrain of Mount Sharp, which required that it alter its path to avoid contact and possible contamination of the site.

A dark, narrow, 100 meter-long streak called lowing downhill on Mars.

This decision was based on the possibility that subsurface water was responsible for the streak, and could be an indication of subsurface life. If slope streaks are indeed linked to seasonal water flows, then proper measures will need to be put in place for future missions, especially crewed ones.

Before we can send astronauts to the surface of Mars, or contemplate creating a permanent human presence there, we need to know where to step and what to avoid!

NASA’s MAVEN Shrinking Its Orbit For Mars 2020 Rover

Aerobraking plan for MAVEN
Aerobraking plan for MAVEN. (left) Current MAVEN orbit around Mars: 6,200 kilometers (~3,850 miles) at highest altitude, and an orbit period of about 4.5 hours. (center) Aerobraking process: MAVEN performs a series of “deep dip” orbits approaching to within about 125 kilometers (~78 miles) of Mars at lowest altitude, causing drag from the atmosphere to slow down the spacecraft. Over roughly 360 orbits spanning 2.5 months, this technique reduces the spacecraft’s altitude to about 4,500 kilometers (~2,800 miles) and its orbit period to about 3.5 hours. (right) Post-aerobraking orbit, with reduced altitude and shorter orbit period. Credits: NASA’s Scientific Visualization Studio/Kel Elkins and Dan Gallagher
› Download in high resolution from the Scientific Visualization Studio

NASA’s 4-year-old atmosphere-sniffing Mars Atmosphere and Volatile Evolution (MAVEN) mission is embarking on a new campaign today to tighten its orbit around Mars. The operation will reduce the highest point of the MAVEN spacecraft’s elliptical orbit from 3,850 to 2,800 miles (6,200 to 4,500 kilometers) above the surface and prepare it to take on additional responsibility as a data-relay satellite for NASA’s Mars 2020 rover, which launches next year.

“The MAVEN spacecraft has done a phenomenal job teaching us how Mars lost its atmosphere and providing other important scientific insights on the evolution of the Martian climate,” said Jim Watzin, director of NASA’s Mars Exploration Program. “Now we’re recruiting it to help NASA communicate with our forthcoming Mars rover and its successors.”

While MAVEN’s new orbit will not be drastically shorter than its present orbit, even this small change will significantly improve its communications capabilities. “It’s like using your cell phone,” said Bruce JakoskyMAVENprincipal investigator from the University of Colorado, Boulder. “The closer you are to a cell tower, the stronger your signal.”

A strong telecommunications antenna signal is not the only benefit of a tighter orbit. Coming in nearly 1,000 miles (about 1,500 kilometers) closer also will allow the MAVEN orbiter to circle Mars more frequently – 6.8 orbits per Earth day versus 5.3 previously – and thus communicate with the Mars rovers more frequently. While not conducting relay communications, MAVEN will continue to study the structure and composition of the upper atmosphere of Mars. “We’re planning a vigorous science mission far into the future,” Jakosky said.

The MAVEN mission was designed to last two years in space, but the spacecraft is still operating normally. With the mission managing its fuel to last through 2030, NASA plans to use MAVEN’s relay capability as long as possible. The MAVEN orbiter carries an ultra-high-frequency radio transceiver – similar to transceivers carried on other Mars orbiters – that allows it to relay data between Earth and rovers or landers on Mars. The MAVEN spacecraft already has served occasionally as NASA’s communication liaison with the Curiosity rover.

Over the next few months, MAVEN engineers will use a navigation technique known as aerobraking – like applying the brakes on a car – to take advantage of the drag of the Red Planet’s upper atmosphere to slow the spacecraft down gradually, orbit by orbit. This is the same drag you would feel if you put your hand out of the window of a moving car.

Based on the tracking of the spacecraft by the navigation team at NASA’s Jet Propulsion Laboratory in Pasadena, California, and at Lockheed Martin in Littleton, Colorado, engineers will begin carefully lowering the lowest part of the spacecraft’s orbit into the Martian upper atmosphere over the next couple of days by firing its thrusters. The spacecraft will circle Mars at this lower altitude about 360 times over the next 2.5 months, slowing down slightly with each pass through the atmosphere. While it may seem like a time-consuming process, aerobraking is the most efficient way to change the spacecraft’s trajectory, said Jakosky: “The effect is the same as if we fired our thrusters a little bit on every orbit, but this way, we use very little fuel.”

Fortunately, the team has ample experience operating the spacecraft at these lower altitudes. On nine previous occasions throughout the mission, MAVEN engineers have dipped the orbiter into the same altitude targets for aerobraking to take measurements of the Martian atmosphere. As a result of these “deep dips” and other measurements, NASA has learned that solar wind and radiation had stripped Mars of most of its atmosphere, changing the planet’s early climate from warm and wet to the dry environment we see today. MAVEN also discovered two new types of auroras on Mars and the presence of charged metal atoms in its upper atmosphere that tell us that a lot of debris is hitting Mars that may affect its climate.

MAVEN’s principal investigator is based at the University of Colorado’s Laboratory for Atmospheric and Space Physics, Boulder. The university provided two science instruments and leads science operations, as well as education and public outreach, for the mission. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN project and provided two science instruments for the mission. Lockheed Martin built the spacecraft and is responsible for mission operations. The University of California at Berkeley’s Space Sciences Laboratory also provided four science instruments for the mission. NASA’s Jet Propulsion Laboratory in Pasadena, California, provides navigation and Deep Space Network support, as well as the Electra telecommunications relay hardware and operations.

For more information on the MAVEN mission, visit:

https://www.nasa.gov/maven or http://lasp.colorado.edu/home/maven/

For more information on the Mars 2020 mission, visit:

https://mars.nasa.gov/mars2020/
News Media Contact

Nancy Jones
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-0039
nancy.n.jones@nasa.gov

DC Agle
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-9011
agle@jpl.nasa.gov

Story by:
Lonnie Shekhtman
NASA’s Goddard Space Flight Center

2019-020