Skip to main content

A New Explanation for Why Mars is Red

Well that’s ruined all my lectures! I’ve spent years talking about space and a go to fact is the red colour of Mars. It’s been long believed that it was caused by the same chemical process that creates rust on Earth, a new paper suggests this is not the case! The team of researchers simulated conditions of Mars in a lab and now think a chemical called ferrihydrite, an iron oxide that contains water. It now looks like the planet’s characteristic red colour is due to a time when Mars was covered in water! 

Mars, often called the Red Planet is the fourth planet from the Sun. With a thin atmosphere composed mostly of carbon dioxide, Mars features a stark landscape of vast plains, huge volcanoes including Olympus Mons (the largest in our solar system), and deep canyons like Valles Marineris. Its surface has evidence of ancient rivers and lakes, suggesting Mars once had conditions that could have been suitable for microbial life. Its extreme temperature changes and frequent global dust storms are typical of this harsh world. 

Mars seen before, left, and during, right, a global dust storm in 2001. Credit: NASA/JPL/MSSS

The distinctive red colour goes back centuries; the ancient Egyptians called Mars ‘Her Desher’ which translates to ‘the Red One’, the Romans named it after the God of war and the Chinese called it ‘the fire star.’ Even Babylonian records that go back to 2000 BC noted its red colour. In 1610, when Galileo first observed Mars through a telescope, he confirmed its planetary nature but also noted a more red/brown hue. This was largely due to the poor quality optics of the day and it wasn’t until optics improved that its red colour was observed in all its glory.

A bust of Galileo at the Galileo Museum in Florence, Italy. The museum is displaying recovered parts of his body. Credit Kathryn Cook for The New York Times

A team of researchers led by Dr Adomas Valantinas from Brown University in USA have published a paper in Nature Communications that has analysed the red colouration of Mars and challenge the common view that it’s a rust like material that is responsible. They used data from a number of different Mars missions from NASA’s Reconnaissance Orbiter to ESA’s Mars Express and ExoMars (which has the Colour and Stereo Surface Imaging System onboard.) The data from the orbiters was supported by data from various rovers too and further supplemented by analysis of artificial Mars-like materials in a laboratory.

Mars Express, which is now studying Phobos.
An artist’s illustration of the Mars Express Orbiter above Mars. Its MARSIS instrument has been updated so it can study the moon Phobos. Image Credit: Spacecraft: ESA/ATG medialab; Mars: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO

The analysis, which included experiments and measurements at the University of Grenoble, Brown University and the University of Winnipeg revealed the presence of Ferrihydrite. Not only was it present in the Martian dust, it seemed to be widespread across the Martian landscape. Ferriydrite is an oxyhydroxide mineral (one that contains oxygen, hydrogen and at least one metal.)

The widespread discovery of ferrihydrite on in Martian dust helps us to understand more about the geological history of Mars and its potential habitability. The existence of the ferrihydrite tells us that there were once cooler, wet conditions on Mars since that is a neccessity for the formation of the mineral. It’s an exciting discovery because its one more reason to believe that Mars was once a hospitable world. 

The team are keen to learn more and are now waiting for Martian samples to study directly and for that, they are waiting for the Perseverance rover. It has been systematically collecting core samples of Martian soil from the Jezero Crater and storing them in titanium tubes ready for transport home. Once the team has these, they will be able to check whether their theory about ferrihydrite is correct.

Source : Why Mars could be red

The post A New Explanation for Why Mars is Red appeared first on Universe Today.



from Universe Today https://ift.tt/asxF5WZ
via IFTTT

Comments

Popular posts from this blog

More Data and Machine Learning has Kicked SETI Into High Gear

For over sixty years, astronomers and astrophysicists have been engaged in the Search for Extraterrestrial Intelligence (SETI). This consists of listening to other star systems for signs of technological activity (or “technosignatures), such as radio transmissions. This first attempt was in 1960, known as Project Ozma, where famed SETI researcher Dr. Frank Drake (father of the Drake Equation) and his colleagues used the Robert C. Byrd Green Bank Telescope in West Virginia to conduct a radio survey of Tau Ceti and Epsilon Eridani. Since then, the vast majority of SETI surveys have similarly looked for narrowband radio signals since they are very good at propagating through interstellar space. However, the biggest challenge has always been how to filter out radio transmissions on Earth – aka. radio frequency interference (RFI). In a recent study, an international team led by the Dunlap Institute for Astronomy and Astrophysics (DIAA) applied a new deep-learning algorithm to data collecte...

The First Close-Up Picture of Star Outside the Milky Way

Like a performer preparing for their big finale, a distant star is shedding its outer layers and preparing to explode as a supernova. Astronomers have been observing the huge star, named WOH G64, since its discovery in the 1970s. It’s one of the largest known stars, and also one of the most luminous and massive red supergiants (RSGs). The star is surrounded by an envelope of expelled star-stuff, which could indicate it’s getting ready to explode. WOH G64 isn’t in the Milky Way; it’s in the Large Magellanic Cloud (LMC), the Milky Way’s largest satellite galaxy. Getting these detailed image is quite a feat for the ESO’s Very Large Telescope Interferometer. It’s also quite an accomplishment for the team of scientists behind the image. They’ve published their images and the results of their observations of the star in the journal Astronomy and Astrophysics. Their research is titled “ Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic ...

eROSITA Sees Changes in the Most Powerful Quasar

After almost seventy years of study, astronomers are still fascinated by active galactic nuclei (AGN), otherwise known as quasi-stellar objects (or “quasars.”) These are the result of supermassive black holes (SMBHs) at the center of massive galaxies, which cause gas and dust to fall in around them and form accretion disks. The material in these disks is accelerated to close to the speed of light, causing it to release tremendous amounts of radiation in the visible, radio, infrared, ultraviolet, gamma-ray, and X-ray wavelengths. In fact, quasars are so bright that they temporarily outshine every star in their host galaxy’s disk combined. The brightest quasar observed to date, 100,000 billion times as luminous as our Sun, is known as SMSS J114447.77-430859.3 (J1144). This AGN is hosted by a galaxy located roughly 9.6 billion light years from Earth between the constellations Centaurus and Hydra. Using data from the eROSITA All Sky Survey and other space telescopes, an international t...