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This image from NASA's Mars rover Curiosity shows a small bright object on the ground beside the rover at the 'Rocknest' site. The rover team has assessed this object as debris from the spacecraft, possibly from the events of landing on Mars.
This image from NASA's Mars rover Curiosity shows a small bright object on the ground beside the rover at the 'Rocknest' site. The rover team has assessed this object as debris from the spacecraft, possibly from the events of landing on Mars.

Small Debris on the Ground Beside Curiosity

Small spherical objects fill the field in this mosaic combining four images from the Microscopic Imager on NASA's Mars Exploration Rover Opportunity at an outcrop called 'Kirkwood' in the Cape York segment of the western rim of Endeavour Crater.
Small spherical objects fill the field in this mosaic combining four images from the Microscopic Imager on NASA's Mars Exploration Rover Opportunity at an outcrop called 'Kirkwood' in the Cape York segment of the western rim of Endeavour Crater.

Puzzling Little Martian Spheres That Don't Taste Like 'Blueberries'

This image of a target called 'Private Joseph Field' combines four images from the microscopic imager on the robotic arm of NASA's Mars Exploration Rover Opportunity, with enhanced color information added from the rover's panoramic camera.
This image of a target called 'Private Joseph Field' combines four images from the microscopic imager on the robotic arm of NASA's Mars Exploration Rover Opportunity, with enhanced color information added from the rover's panoramic camera.

Opportunity View of 'Private Joseph Field' on Mars

This image from NASA's 2001 Mars Odyssey spacecraft shows a region of the south pole where the surface has developed linear markings, a pattern not unlike a thumbprint.
This image from NASA's 2001 Mars Odyssey spacecraft shows a region of the south pole where the surface has developed linear markings, a pattern not unlike a thumbprint.

South Polar Surface

A sand sheet and dune forms are present on the floor of Capri Chasmain this image from NASA's 2001 Mars Odyssey spacecraft.
A sand sheet and dune forms are present on the floor of Capri Chasmain this image from NASA's 2001 Mars Odyssey spacecraft.

Capri Chasma

Modern-day Mars experiences cyclical changes in climate and, consequently, ice distribution. Unlike Earth, the obliquity (or tilt) of Mars changes substantially on timescales of hundreds of thousands to millions of years.
Modern-day Mars experiences cyclical changes in climate and, consequently, ice distribution. Unlike Earth, the obliquity (or tilt) of Mars changes substantially on timescales of hundreds of thousands to millions of years.

Changes in Tilt of Mars' Axis

This 360-degree view, called the 'McMurdo' panorama, comes from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as 'Low Ridge.'
This 360-degree view, called the 'McMurdo' panorama, comes from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as 'Low Ridge.'

'McMurdo' Panorama from Spirit's 'Winter Haven'

This mosaic of images shows the soil in front of NASA's Mars Exploration Rover Spirit after a series of short backward drives during attempts to extricate the rover from a sand trap in January and early February 2010.
This mosaic of images shows the soil in front of NASA's Mars Exploration Rover Spirit after a series of short backward drives during attempts to extricate the rover from a sand trap in January and early February 2010.

Soil Disturbed by Spirit Drives Before Fourth Martian Winter (False Color)

The arc of hills in this image from NASA's Mars Reconnaissance Orbiter spacecraft is the rim of an old and infilled impact crater. The sediments that were deposited within the crater have since formed polygonal cracks.
The arc of hills in this image from NASA's Mars Reconnaissance Orbiter spacecraft is the rim of an old and infilled impact crater. The sediments that were deposited within the crater have since formed polygonal cracks.

A Frost Enhanced Landscape

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.

Candor Chasma - False Color

Dark slope streaks mark the inner rim of this unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks mark the inner rim of this unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

This image captured by NASA's Mars Reconnaissance Orbiter is of an ancient, approximately 3 billion year-old landslide shows two distinct surface albedos, which are proportions of reflected light.
This image captured by NASA's Mars Reconnaissance Orbiter is of an ancient, approximately 3 billion year-old landslide shows two distinct surface albedos, which are proportions of reflected light.

Hydrated Sulfate Landslides in Ophir Chasma

This frame from a video clip shows moments during a demonstration of drilling into a rock at NASA's JPL, Pasadena, Calif., with a test double of the Mars rover Curiosity. The drill combines hammering and rotation motions of the bit.
This frame from a video clip shows moments during a demonstration of drilling into a rock at NASA's JPL, Pasadena, Calif., with a test double of the Mars rover Curiosity. The drill combines hammering and rotation motions of the bit.

Video Clip of a Rover Rock-Drilling Demonstration at JPL

The wind eroded material in this image from NASA's 2001 Mars Odyssey spacecraft are located just north of Amazonis Mensa.
The wind eroded material in this image from NASA's 2001 Mars Odyssey spacecraft are located just north of Amazonis Mensa.

Wind Erosion

NASA's Mars Exploration Rover Opportunity used its microscopic imager to record this close-up view of texture on part of a rock informally named
NASA's Mars Exploration Rover Opportunity used its microscopic imager to record this close-up view of texture on part of a rock informally named

Magnified View of Texture on Part of 'Tisdale 2' Rock

This image comes from observations of Horowitz crater by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter. The features that extend down the slope during warm seasons are called recurring slope lineae.
This image comes from observations of Horowitz crater by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter. The features that extend down the slope during warm seasons are called recurring slope lineae.

Warm-Season Flows on Slope in Horowitz Crater (Eight-Image Sequence)

This picture from NASA's Curiosity rover puts a color view obtained by the rover in the context of a computer simulation derived from images acquired from orbiting spacecraft. The view looks north, showing the distant ridge of Gale Crater.
This picture from NASA's Curiosity rover puts a color view obtained by the rover in the context of a computer simulation derived from images acquired from orbiting spacecraft. The view looks north, showing the distant ridge of Gale Crater.

Curiosity's Landscape Portrait in Context

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the delta deposit in Eberswalde Crater.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the delta deposit in Eberswalde Crater.

Eberswalde Crater - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Daedalia Planum as well as several windstreaks.

Daedalia Planum Windstreaks

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Eos Chasma.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Eos Chasma.

Eos Chasma - False Color

The steep feature in this image from NASA's 2001 Mars Odyssey spacecraft is the margin of the north polar cap, called Olympia Rupes.
The steep feature in this image from NASA's 2001 Mars Odyssey spacecraft is the margin of the north polar cap, called Olympia Rupes.

Olympia Rupes

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Proctor Crater.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Proctor Crater.

Proctor Crater Dunes - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows Gasa Crater, a small crater within a larger crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows Gasa Crater, a small crater within a larger crater.

Gasa Crater

This image from NASA's Mars Reconnaissance Orbiter shows cones with summit pits that are very similar to cinder cones on Earth. They are also very well-preserved, peppered by only small impact craters, so they must be geologically young.
This image from NASA's Mars Reconnaissance Orbiter shows cones with summit pits that are very similar to cinder cones on Earth. They are also very well-preserved, peppered by only small impact craters, so they must be geologically young.

Recent Volcanism in Valles Marineris

This unnamed channel is located east of Baetis Chaos as seen by NASA's 2001 Mars Odyssey spacecraft.
This unnamed channel is located east of Baetis Chaos as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

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