New Discovery: Frost Forms on Mars' Tallest Volcanoes in Tharsis Region

Mars, Tharsis region Montserrat
Approximately 150,000 tonnes of water condense daily during colder seasons
Challenges understanding of Mars' climate processes and offers new insights into the planet's water cycle
Discovered using data from ESA's Trace Gas Orbiter and Mars Express orbiter
Frost covers vast area despite being thin (likely one-hundredth of a millimetre thick)
Frost forms on Mars' tallest volcanoes in Tharsis region
Observed on Olympus Mons and Pavonis Mons, three times as tall as Mount Everest
New Discovery: Frost Forms on Mars' Tallest Volcanoes in Tharsis Region

Mars, the fourth planet from the sun, is known for its volcanic activity and harsh climate. Recently, an intriguing discovery was made regarding some of Mars' largest mountains in the Tharsis region near the equator. Early morning frost has been observed on these colossal Martian volcanoes, including Olympus Mons and Pavonis Mons, which are three times as tall as Mount Everest. This frost appears as a bluish hue on the caldera floors and is absent from well-lit slopes.

The discovery was made using data from the European Space Agency's (ESA) Trace Gas Orbiter (TGO) and Mars Express orbiter. The researchers, led by Adomas Valantinas of the University of Berne in Switzerland and Brown University in the US, calculated that during colder Martian seasons, approximately 150,000 tonnes of water condense daily on the tops of these towering mountains.

Frost has been found to form overnight on the summit craters and sections of their rims. Despite being exceptionally thin (likely only one-hundredth of a millimetre thick), it covers a vast area. The researchers suggest that Martian winds may blow up the mountainsides, carrying relatively moist air into the calderas where it condenses and settles as frost.

This discovery is significant because scientists previously believed that frost could not form on the Tharsis volcano tops due to high daytime temperatures and thin atmospheric conditions. However, this finding challenges our understanding of Mars' climate processes and offers new insights into the planet's water cycle.

The Tharsis region is home to a dozen large volcanoes, including Pavonis Mons and Olympus Mons. These extinct volcanoes rise through Mars' thin atmosphere, with Olympus Mons being the largest in both diameter (600 kilometers or 370 miles) and height (around 25 kilometers or 15.5 miles).

The discovery of water frost on Mars' highest volcanoes adds to the ongoing success of ESA's ExoMars and Mars Express missions, which have provided valuable data about the Red Planet's geology, atmosphere, and potential for past or present life.



Confidence

90%

Doubts
  • Are there any potential alternative explanations for the observed frost?
  • Is the amount of water condensing daily an accurate measurement?

Sources

100%

  • Unique Points
    • Early morning frost has been spotted on some of Mars' largest mountains near the equator.
    • Frost appears as a bluish hue on the caldera floors and is absent from well-lit slopes.
    • In colder months, approximately 150,000 tonnes of water condense daily on the tops of these towering mountains.
  • Accuracy
    No Contradictions at Time Of Publication
  • Deception (100%)
    None Found At Time Of Publication
  • Fallacies (100%)
    None Found At Time Of Publication
  • Bias (100%)
    None Found At Time Of Publication
  • Site Conflicts Of Interest (100%)
    None Found At Time Of Publication
  • Author Conflicts Of Interest (100%)
    None Found At Time Of Publication

100%

  • Unique Points
    • The discovery was made using TGO’s CaSSIS instrument and confirmed by looking again at the area using TGO’s NOMAD spectrometer and Mars Express’ HRSC.
    • Frost has been found for the first time near Mars’ equator.
    • Despite being thin (likely only one-hundredth of a millimetre thick), they cover a vast area and represent about 150,000 tonnes of water swapping between surface and atmosphere each day during the cold seasons.
    • The discovery relied upon collaboration between ExoMars TGO and Mars Express.
  • Accuracy
    No Contradictions at Time Of Publication
  • Deception (100%)
    None Found At Time Of Publication
  • Fallacies (100%)
    None Found At Time Of Publication
  • Bias (100%)
    None Found At Time Of Publication
  • Site Conflicts Of Interest (100%)
    None Found At Time Of Publication
  • Author Conflicts Of Interest (0%)
    None Found At Time Of Publication

99%

  • Unique Points
    • Mars volcanos in the Tharsis region, including Olympus Mons, Arsia Mons, Pavonis Mons, and Ascraeus Mons, have water ice frost.
    • Frost settles in the shadowed regions of calderas where temperatures are colder.
    • Winds bring relatively moist air from near the surface up to higher altitudes, where it condenses and settles as frost.
  • Accuracy
    No Contradictions at Time Of Publication
  • Deception (100%)
    None Found At Time Of Publication
  • Fallacies (95%)
    The author makes several statements that are not fallacious. However, there is an instance of an appeal to authority when the authors quote Adomas Valantinas and Nicolas Thomas. The author also uses some inflammatory rhetoric by stating 'we thought it was impossible' and 'hints that there are exceptional processes at play'. These statements do not provide any new information or evidence, but rather attempt to create a sense of excitement or wonder about the discovery. However, these instances do not significantly impact the overall quality of the article.
    • ]We thought it was impossible for frost to form around Mars[apos]s equator,
  • Bias (100%)
    None Found At Time Of Publication
  • Site Conflicts Of Interest (100%)
    None Found At Time Of Publication
  • Author Conflicts Of Interest (100%)
    None Found At Time Of Publication

98%

  • Unique Points
    • Water frost has been discovered for the first time near Mars equator.
    • Despite being incredibly thin, with a thickness equivalent to that of a human hair, the frost covers a vast area and its water content could fill roughly 60 Olympic swimming pools.
    • Frost deposition is linked to colder Martian seasons, making the window for spotting it even narrower.
    • Mars low atmospheric pressure creates an unfamiliar situation on the Red Planet, but moist air blowing up mountain slopes can still condense into frost.
  • Accuracy
    No Contradictions at Time Of Publication
  • Deception (100%)
    None Found At Time Of Publication
  • Fallacies (92%)
    None Found At Time Of Publication
  • Bias (100%)
    None Found At Time Of Publication
  • Site Conflicts Of Interest (100%)
    None Found At Time Of Publication
  • Author Conflicts Of Interest (100%)
    None Found At Time Of Publication