Water in space: Evidence of flowing liquid water on Mars

Mountain on Mars that contains flowing water.

Image credit: NASA/JPL/University of Arizona/Public domain.

First published on 29th September 2015. Last updated on 5th August 2017 by Dr Helen Klus

1. Flowing liquid water on Mars

In September 2015, NASA announced that they've found evidence of liquid water currently flowing on Mars[1].

This began with the discovery of dark streaks on the sides of several craters[2]. These are up to a few hundred meters long, and appear seasonally. They form when it's ‘warm', at over -10 °C, and disappear when it is colder. These were found using the HiRISE (High Resolution Imaging Science Experiment) camera attached to NASA's Mars Reconnaissance Orbiter (MRO) spacecraft, which was launched in 2005, and attained Martian orbit in 2006.

A team led by Lujendra Ojha found hydrated salts in these regions using data from the MRO's CRIS (Compact Reconnaissance Imaging Spectrometer)[3]. These salts are only present when the streaks are, and so it's thought that the streaks must be caused by flowing salt water.

Animation showing dark streaks on the side of the mountain gradually moving.

Animation of flowing water in the Hale Crater on Mars, image created using data from NASA's Mars Reconnaissance Orbiter spacecraft. Image credit: JPLraw/Public domain.

Dark streaks on the inside of a Crater on Mars.

Dark streaks on the side of the Garni Crater on Mars, image created using data from NASA's Mars Reconnaissance Orbiter spacecraft. Image credit: JPLraw NASA/JPL-Caltech/Univ. of Arizona/Public domain.

Over 25 spacecraft have been to Mars since the 1960s. Evidence for water on Mars was first found by NASA's Mariner 9, which launched in 1971. Data from Mariner 9 showed that Mars had once contained rivers, which had led to the formation of large, complex canyons. Data from NASA's Viking 1 and Viking 2, which launched in 1975, showed that Mars once contained both rain and oceans.

Data from NASA's Mars Global Surveyor and Mars Pathfinder, indicated that Mars may have once have been warm and wet, with flowing water, and NASA's 2001 Mars Odyssey orbiter found evidence of frozen water on the Martian surface.

The European Space Agency's (ESA) Mars Express confirmed the presence of frozen water and carbon dioxide at the Martian poles, and NASA's Opportunity Rover found rocks that are thought to have once been underwater in a salty sea.

There are a number of landers and orbiters currently on Mars, and many new missions to Mars are in progress. But Mars is not the only place outside of Earth to contain water.

Water is very common in the universe because hydrogen and oxygen are both reactive and abundant. Hydrogen is the most common element in the universe, and was created in the big bang, and oxygen is a fairly common element made inside of stars.

2. Water elsewhere in the Solar System

Water has been found in trace amounts on many moons, and on every planet in the Solar System[4a][5]. Frozen water exists at the bottom of deep craters on Mercury's poles[6] and on the Moon[7]. Venus is thought to have once contained oceans[8], and it's thought that oceans currently exist below the frozen surface of at least three of Jupiter's moons, at least two of Saturn's moons, and possibly on Neptune's moon Triton. There may also be subsurface oceans on dwarf planets Ceres and Pluto[4b].

The majority of water in the Solar System resides in comets, which orbit the Sun from the Kuiper belt and the Oort cloud. The Kuiper belt is thought to be composed of about a trillion comets[9], and the Oort cloud may contain up to 2 trillion[10]. In total, these may contain tens of thousands of times the amount of water in the Earth's oceans*.

Amino acids – the ‘building blocks of life' – have also been found inside comets, and it's possible that both water and amino acids were transported to Earth and other planets when they were bombarded with comets during the formation of the Solar System[11].

Further evidence of liquid water in the Jupiter system may come from NASA's Juno spacecraft, which lunched in 2011, and will arrive at Jupiter in 2017. Juno will look for water in Jupiter's atmosphere. The ESA plan to launch a mission to Jupiter's moons, Ganymede, Callisto, and Europa, in 2022. All of these moons are thought to contain oceans. This mission is known as Jupiter Icy Moon Explorer (JUICE), and should arrive at Jupiter in 2030. NASA also plan to launch a mission to Jupiter's moons in the 2020s, known as the Europa Multiple-Flyby Mission. This will focus on looking for evidence of life on Europa.

Further evidence of liquid water in the Saturn system may come from the Cassini spacecraft, which launched in 1997, and is currently in orbit around Saturn. Data from the Cassini spacecraft, and its lander, the Huygens probe, have already shown that water exists on two of Saturn's moons, Titan and Enceladus. Titan was found to have sand dunes, coastlines, islands, and mountains, and Enceladus was found to erupt in geysers that can send water into orbit around Saturn. In September 2015, data from Cassini was used to show that Enceladus might also contain a global ocean[12] that:

...could contain environments suitable for living organisms[13].

Evidence of water in the Kuiper belt may come from NASA's New Horizons mission. New Horizons passed Pluto in July 2015. Scientists were surprised to discover that it may contain liquid water, and we'll know more about why this is as information is transmitted back to Earth. It's hoped that the New Horizons spacecraft will be able to give us similar information about at least one more Kuiper belt object.

3. Water outside of the Solar System

Water has also been observed outside of the Solar System, in molecular clouds[14], protoplanetary discs[15], exocomets[16], and in the atmospheres of exoplanets[17].

Painting of a ring of water on the outside of a disc of hot dust surrounding a star.

Artist's impression of the TW Hydrae system, a protoplanetary disc that contains ‘oceans of water'. Image credit: NASA/JPL-Caltech/Public domain.

Scientists are most interested in looking for liquid water, as this is thought to be essential for the formation of life. For liquid water to exist on a planet, it must be far enough away from its star so that the water doesn't boil away, but close enough that it doesn't freeze. This area is known as the habitable zone, and it's currently thought that there could be tens of billions of planets in the Milky Way that exist within the habitable zone[18].

At least 30 have already been identified[19], including ‘water world' GJ 1214b[20]. There are numerous missions that may provide further evidence of water outside of the Solar System.

We are beginning to discover that water is everywhere in the universe, and where there is water, there may be life.

Painting of two aliens under water.

Sardu Reef. Image credit: Alex Ries, 2012/Copyrighted, used with permission.

Total mass of water in a comet = 1013 kg.

Total mass of water in Earth's oceans = 1.4×1021 kg.

Total mass of water in a comet × number of comets = 1013 × 3×1012 = 3×1025 kg.

Water in comets/Water in the oceans
3×1025 kg/1.4×1021 kg
= 21,429.

UPDATE: As of 2017, 52 exoplanets have been discovered within the habitable zone. In 2016, astronomers at the University of California, Santa Cruz found evidence of clouds of water around the brown dwarf WISE 0855. Brown dwarfs are objects that are much larger than planets, but are slightly too small to become stars.

4. References

  1. NASA, 'NASA Confirms Evidence That Liquid Water Flows on Today's Mars', last accessed 01-06-17.

  2. NASA, 'Dark, Recurring Streaks on Walls of Garni Crater on Mars', last accessed 01-06-17.

  3. Ojha, L., et al, 2015, 'Spectral evidence for hydrated salts in recurring slope lineae on Mars', Nature Geoscience, 8, pp.829-832.

  4. (a, b) NASA, 'The Solar System and Beyond is Awash in Water', last accessed 01-06-17.

  5. NASA, 'Venus: In Depth', last accessed 01-06-17.

  6. NASA, 'MESSENGER Finds New Evidence for Water Ice at Mercury's Poles', last accessed 01-06-17.

  7. NASA, 'NASA-Funded Scientists Detect Water on Moon's Surface that Hints at Water Below', last accessed 01-06-17.

  8. Dorminey, B., 2009, 'Venus may have had continents and oceans', Nature News, last accessed 01-06-17.

  9. NASA, 'Kuiper Belt: In Depth', last accessed 01-06-17.

  10. NASA, 'Kuiper Belt and Oort Cloud', last accessed 01-06-17.

  11. NASA, 'NASA Researchers Make First Discovery of Life's Building Block in Comet', last accessed 01-06-17.

  12. NASA, 'Cassini Finds Global Ocean in Saturn's Moon Enceladus', last accessed 01-06-17.

  13. NASA, 'Spacecraft Data Suggest Saturn Moon's Ocean May Harbor Hydrothermal Activity', last accessed 01-06-17.

  14. NASA Astrobiology Institute, 'Cold Clouds and Water in Space', last accessed 01-06-17.

  15. NASA, 'Herschel Finds Oceans of Water in Disk of Nearby Star', last accessed 01-06-17.

  16. NASA Spitzer Space Telescope, 'It's Raining Comets', last accessed 01-06-17.

  17. NASA, 'NASA Telescopes Find Clear Skies and Water Vapor on Exoplanet', last accessed 01-06-17.

  18. ESO, 'Many Billions of Rocky Planets in the Habitable Zones around Red Dwarfs in the Milky Way', last accessed 01-06-17.

  19. The Planetary Habitability Laboratory, 'Habitable Exoplanets Catalog', last accessed 01-06-17.

  20. NASA, 'Hubble Discovers Waterworld Planet', last accessed 01-06-17.

Back to top

The Star Garden is a science news and science education website run by Dr Helen Klus.

How we came to know the cosmos covers the history of physics focusing on space and time, light and matter, and the mind. It explains the simple discoveries we made in prehistoric times, and how we built on them, little by little, until the conclusions of modern theories seem inevitable. This is shown in a timeline of the universe.

The Star Garden covers the basics for KS3, KS4, and KS5 science revision including SATs, GCSE science, and A-level physics.