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MGS/TES June-August Sequence

MGS/TES June-August Sequence

About the Object

  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    At the 2001 Mars opposition, the planet was approximately 43 million miles (68 million km) from Earth.
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    The planet has a diameter of 4,222 miles (6,794 km) at the equator.

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    Principal Scientists: P. Christensen (Arizona State University)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    Mars Global Surveyor (MGS)>Thermal Emission Spectrometer (TES)
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    June 17 - August 26, 2001
  • Filters
    FiltersThe camera filters that were used in the science observations.
    Infrared wavelengths: 2.3 - 15.4nm
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Mars
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planet, Global Dust Storm
  • Release Date
    October 11, 2001
  • Science Release
    Scientists Track “Perfect Storm” on Mars
  • Credit
    Philip Christensen (Arizona State University) and the TES Team

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov