Saturn and Mars Team Up to Make Their Closest Approaches to Earth in 2018

Stsci_2018-29f_1024

stsci_2018-29f July 26th, 2018

Credit: NASA and ESA

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 with summer in the northern hemisphere. The picture on the right, taken on July 18, 2018, features a global dust storm, with summer in the southern hemisphere.

Scientist believe that heat from the southern hemisphere’s 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.

Provider: Space Telescope Science Institute

Image Source: https://hubblesite.org/contents/news-releases/2018/news-2018-29

Curator: STScI, Baltimore, MD, USA

Image Use Policy: http://hubblesite.org/copyright/

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Image Details Image Details

Image Type
Observation
Object Name
Mars
Subject - Solar System
Planet > Satellite

Position Details Position Details

Position (ICRS)
RA = 1h 14m 3.1s
DEC = -22° 22’ 19.2”
Constellation
Cetus

Color Mapping Details Color Mapping

  Telescope Spectral Band Wavelength
Purple Hubble (WFC3/UVIS) Optical (UV wide) 275.0 nm
Blue Hubble (WFC3/UVIS) Optical (v) 410.0 nm
Green Hubble (WFC3/UVIS) Optical (OIII) 502.0 nm
Red Hubble (WFC3/UVIS) Optical (SII) 673.0 nm
Spectrum_base
Purple
Blue
Green
Red
Stsci_2018-29f_1280
×
ID
2018-29f
Subject Category
A.1.4  
Subject Name
Mars
Credits
NASA and ESA
Release Date
2018-07-26T00:00:00
Lightyears
Redshift
Reference Url
https://hubblesite.org/contents/news-releases/2018/news-2018-29
Type
Observation
Image Quality
Good
Distance Notes
Facility
Hubble, Hubble, Hubble, Hubble
Instrument
WFC3/UVIS, WFC3/UVIS, WFC3/UVIS, WFC3/UVIS
Color Assignment
Purple, Blue, Green, Red
Band
Optical, Optical, Optical, Optical
Bandpass
UV wide, v, OIII, SII
Central Wavelength
275, 410, 502, 673
Start Time
Integration Time
Dataset ID
Notes
Coordinate Frame
ICRS
Equinox
Reference Value
18.5128131, -22.3719889
Reference Dimension
Reference Pixel
Scale
Rotation
Coordinate System Projection:
Quality
Position
FITS Header
Notes
Creator (Curator)
STScI
URL
http://hubblesite.org
Name
Space Telescope Science Institute Office of Public Outreach
Email
outreach@stsci.edu
Telephone
410-338-4444
Address
3700 San Martin Drive
City
Baltimore
State/Province
MD
Postal Code
21218
Country
USA
Rights
http://hubblesite.org/copyright/
Publisher
STScI
Publisher ID
stsci
Resource ID
STSCI-H-p1829f-f-4529x2400.tif
Metadata Date
2021-10-04T17:22:19-04:00
Metadata Version
1.2
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