What was recently found on mars




















These factors combine to increase the likelihood of life on the planet at some point in time, as well as indicating that there is potential for the planet to be increasingly hospitable to future human exploration.

The second announcement from the space agency was regarding methane, first detected in the Martian atmosphere by Curiosity in Methane is the simplest organic molecule and is perhaps best known as a greenhouse gas here on Earth. Or so went the theories of an enthusiastic band of pre-schoolers as reported by their teacher. Were they correct? Well, yes! And no. The number of craters on Mars varies dramatically from place to place, depending on how old the surface is. Much of the surface of the southern hemisphere is extremely old, and so has many craters — including the planet's largest, 1,mile-wide 2, km Hellas Planitia — while that of northern hemisphere is younger and so has fewer craters.

Some volcanoes also have just a few craters, which suggests they erupted recently, with the resulting lava covering up any old craters. Some craters have unusual-looking deposits of debris around them resembling solidified mudflows, potentially indicating that the impactor hit underground water or ice. In , the European Space Agency's Mars Express spacecraft detected what could be a slurry of water and grains underneath icy Planum Australe. Some reports describe it as a "lake," but it's unclear how much regolith is inside the water.

This body of water is said to be about Its underground location is reminiscent of similar underground lakes in Antarctica, which have been found to host microbes. Vast deposits of what appear to be finely layered stacks of water ice and dust extend from the poles to latitudes of about 80 degrees in both Martian hemispheres. These were probably deposited by the atmosphere over long spans of time.

On top of much of these layered deposits in both hemispheres are caps of water ice that remain frozen year-round. Additional seasonal caps of frost appear in the wintertime. These are made of solid carbon dioxide, also known as "dry ice," which has condensed from carbon dioxide gas in the atmosphere. In the deepest part of the winter, this frost can extend from the poles to latitudes as low as 45 degrees, or halfway to the equator.

The dry ice layer appears to have a fluffy texture, like freshly fallen snow, according to a report in the Journal of Geophysical Research-Planets. Mars is much colder than Earth, in large part due to its greater distance from the sun.

The average temperature is about minus 80 degrees Fahrenheit minus 60 degrees Celsius , although it can vary from minus F minus C near the poles during the winter to as much as 70 F 20 C at midday near the equator. The carbon-dioxide-rich atmosphere of Mars is also about times less dense than Earth's on average, but it is nevertheless thick enough to support weather, clouds and winds.

The density of the atmosphere varies seasonally, as winter forces carbon dioxide to freeze out of the Martian air. In the ancient past, the atmosphere was likely significantly thicker and able to support water flowing on the planet's surface.

Over time, lighter molecules in the Martian atmosphere escaped under pressure from the solar wind, which affected the atmosphere because Mars does not have a global magnetic field. NASA's Mars Reconnaissance Orbiter found the first definitive detections of carbon-dioxide snow clouds , making Mars the only body in the solar system known to host such unusual winter weather.

The Red Planet also causes water-ice snow to fall from the clouds. The dust storms on Mars are the largest in the solar system, capable of blanketing the entire Red Planet and lasting for months. One theory as to why dust storms can grow so big on Mars is because the airborne dust particles absorb sunlight, warming the Martian atmosphere in their vicinity.

Warm pockets of air then flow toward colder regions, generating winds. Strong winds lift more dust off the ground, which, in turn, heats the atmosphere, raising more wind and kicking up more dust. These dust storms can pose serious risks to robots on the Martian surface. For example, NASA's Opportunity Mars rover died after being engulfed in a giant storm, which blocked sunlight from reaching the robot's solar panels for weeks at a time. Mars lies farther from the sun than Earth does, so the Red Planet has a longer year — days compared to for our home world.

The two planets have similar day lengths, however; it takes about 24 hours and 40 minutes for Mars to complete one rotation around its axis, versus 24 hours for Earth. The axis of Mars, like Earth's, is tilted in relation to the sun. This means that like Earth, the amount of sunlight falling on certain parts of the Red Planet can vary widely during the year, giving Mars seasons. However, the seasons that Mars experiences are more extreme than Earth's because the Red Planet's elliptical, oval-shaped orbit around the sun is more elongated than that of any of the other major planets.

When Mars is closest to the sun, its southern hemisphere is tilted toward our star, giving the planet a short, warm summer, while the northern hemisphere experiences a short, cold winter. When Mars is farthest from the sun, the northern hemisphere is tilted toward the sun, giving it a long, mild summer, while the southern hemisphere experiences a long, cold winter. Related: How long does it take to get to Mars? The tilt of the Red Planet's axis swings wildly over time because it's not stabilized by a large moon, such as Earth's is.

This situation has led to different climates on the Martian surface throughout its history. A study suggests that the changing tilt also influenced the release of methane into Mars' atmosphere, causing temporary warming periods that allowed water to flow.

The Curiosity rover has previously detected organic molecules buried in Martian sediments, but the new findings add to the list of organic molecules on Mars, further bolstering the case for past habitability.

The rover has 74 cups inside its belly, and nine of those cups are pre-filled with a chemical mixture. The team did not expect the sample to be rich in well-preserved organic molecules since ionizing radiation had long battered the ancient soil.

But after testing the sample with the chemical mixture, the team behind the mission identified organic molecules never before seen on Mars.

The two most significant molecules were benzoic acid and ammonia. The Radiation Assessment Detector RAD instrument on Curiosity found that two forms of radiation pose potential health risks to astronauts in deep space. One is galactic cosmic rays GCRs , particles caused by supernova explosions and other high-energy events outside the solar system. The other is solar energetic particles SEPs associated with solar flares and coronal mass ejections from the sun. NASA will use Curiosity's data to design missions to be safe for human explorers.

Zeitlin, C. Hassler, D. The SAM instrument suite has found Mars' present atmosphere to be enriched in the heavier forms isotopes of hydrogen, carbon, and argon. These measurements indicate that Mars has lost much of its original atmosphere and inventory of water. This loss occurred to space through the top of the atmosphere, a process currently being observed by the MAVEN orbiter. Mahaffy, P.



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