Rubies and Sapphires on Mars?
NASA/JPL-Caltech/UArizona
Rubies and Sapphires on Mars?
ESP_086875_1525  Science Theme: 
This image showcases stunning bedrock outcrops just off the edge of Hellas Basin, one of the largest and deepest well-preserved impact basins on Mars. At first glance, a close-up of the bedrock appears to shimmer with brilliant pink and blue hues, almost like rubies and sapphires. Are our eyes playing tricks on us? Not quite!

If you’re familiar with Mars imagery from HiRISE, you might already have a hunch about what’s happening here. HiRISE captures color images using three broad wavelength filters: blue-green, red, and near-infrared. These are then combined into a red-green-blue (RGB) composite to create what’s known as a “color-infrared” image. You may have heard the term “false color,” but that can be misleading—there’s actually nothing false about it. The issue: human eyes can’t see near-infrared light, but our instruments can, so to help us visualize how bright are dark something is in near-infrared data, we represent the variations in infrared as red, which the human eye can see.

So, if these colorful rocks aren’t gemstones, what are they? Based on other datasets, the pinkish rock would appear white, cream, or perhaps a light grey to our eyes, so this could be a number of other common rock-forming minerals, which has been difficult to nail down with available spectral datasets. The underlying bluish rock, on the other hand, is spectrally consistent with olivine, a mineral that, as its name suggests, is usually olive green.

So, no treasure troves of rubies or sapphires to be found here, but here’s a fun fact: peridot, a variety of olivine, is a semi-precious gemstone and the birthstone for August.

Written by: Livio L. Tornabene, Joe McNeil and Peter Grindrod  (28 April 2025)

 
Acquisition date
06 February 2025

Local Mars time
15:01

Latitude (centered)
-26.992°

Longitude (East)
60.372°

Spacecraft altitude
257.2 km (159.8 miles)

Original image scale range
from 25.9 cm/pixel (with 1 x 1 binning) to 51.9 cm/pixel (with 2 x 2 binning)

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
6.8°

Phase angle
66.7°

Solar incidence angle
62°, with the Sun about 28° above the horizon

Solar longitude
40.6°, Northern Spring

For non-map projected images
North azimuth:  96°
Sub-solar azimuth:  44.7°
JPEG
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

JP2
Black and white
map-projected   (760MB)

IRB color
map-projected   (606MB)

JP2 EXTRAS
Black and white
map-projected  (381MB)
non-map           (581MB)

IRB color
map projected  (203MB)
non-map           (504MB)

Merged IRB
map projected  (228MB)

Merged RGB
map-projected  (215MB)

RGB color
non map           (512MB)
ADDITIONAL INFORMATION
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products
HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

USAGE POLICY
All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible:
NASA/JPL-Caltech/UArizona

POSTSCRIPT
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.