Mars at Opposition (the Elysium Region)
This image is centered near another volcanic region known as Elysium. This area shows many small, dark markings that have been observed by the Hubble telescope and other spacecraft to change as a result of the movement of sand and dust across the Martian surface. In the upper left of this image, at high northern latitudes, a large chevron-shaped area of water ice clouds mark a storm front. Along the right limb, a large cloud system has formed around the Olympus Mons volcano.
Credit:Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical B | 410 nm |
Hubble Space Telescope
WFPC2 |
Optical V | 502 nm |
Hubble Space Telescope
WFPC2 |
Optical R | 673 nm |
Hubble Space Telescope
WFPC2 |