2001 Mars Odyssey
Thermal Emission Imaging System, visible camera
Daylight images in visible light. Good for landforms such as craters, channels and dunes at a few tens of meters per pixel.
- Imaging since
- 2002
- Pixel scale
- 18 to 36 m per pixel
- Credit line
- NASA/JPL-Caltech/Arizona State University
The product this atlas lists
VGEO, visible geometrically projected image (PDS4). Map-projected, so it lines up with a map as it is. The atlas lists the equirectangular version of each observation.
ODE product type: ODY / THEMIS / VGEO4, IDs matching *eqr.
Open one in JMARS
- Open JMARS. It is free from ASU at jmars.mars.asu.edu.
- In the Layer Manager, click Add New Layer, then Stamps, then THEMIS Stamps.
- Expand Image Location Parameters with the down arrow on its right.
- Type the image ID in the Image ID(s) field. Use the observation ID: a letter (V for visible, I for infrared), a 5-character orbit number and a 3-digit image number, for example V98565007. After orbit 99999 the first orbit digit becomes a letter, so VA1466014 is orbit 101466.
- Click OK. The search can take a few minutes.
- Right-click the image outline in the viewing window, then choose to render the image.
From ASU's JMARS documentation, checked 2026-10-08. Not yet run in JMARS by this site. Source: ASU's THEMIS Stamps page.