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Mars Oppositions 2016 and 2018

Mars Oppositions 2016 and 2018

Mars Seen in Clear and Dusty Conditions

These side-by-side images of Mars, taken roughly two years apart, show very different views of the same hemisphere of Mars. Both were captured when Mars was near opposition, which occurs about every two years, when Earth’s orbit catches up to Mars’ orbit. At that time, the Sun, Earth, and Mars fall in a straight line, with Mars and the Sun on “opposing” sides of Earth.

The image on the left, taken on May 12, 2016, shows a clear atmosphere. The picture on the right, taken on July 18, 2018, features a global dust storm, with spring in the southern hemisphere.

Scientists believe that heat from the southern hemisphere’s spring and summer triggers dust storms that originate in the Hellas Basin, the lowest point on the planet.

Although the Red Planet is showing virtually the same face to us, classical dark features first mapped by early sky watchers look different in each image. This is partly because of obscuration from the 2018 global dust storm, but also because the northern hemisphere was tilted toward Earth in 2016, and away from Earth in 2018. The latter view reveals more of southern hemisphere, including the cloud-enshrouded south polar region.

The phenomenon of opposition is a result of the difference in orbital periods between Earth’s orbit and Mars’ orbit. While Earth takes the familiar 365 days to travel once around the Sun, Mars takes 687 Earth days to make its trip around our star. As a result, Earth makes almost two full orbits in the time it takes Mars to make just one, resulting in the occurrence of Martian oppositions about every 26 months.

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.
    The HST observations include those from program 15456 (M. Mutchler)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    July 18, 2018
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F275W, F410M, F502N, F673N
  • 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
  • Release Date
    July 26, 2018
  • Science Release
    Saturn and Mars Team Up to Make Their Closest Approaches to Earth in 2018
  • Credits
    NASA, ESA, and STScI

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Mars Oppositions 2016 and 2018
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

This image is a composite of separate exposures acquired by the WFC3/UVIS instrument. Several filters were used to sample various wavelengths. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Purple: F275W Blue: F410M Green: F502N Red: F673N

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Details

Last Updated
Mar 04, 2025
Contact
Media

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