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Mars Reconnaissance Orbiter Launch Press Kit

MRO launch press kit

August 01, 2005

Download a PDF of the Mars Reconnaissance Orbiter Launch Press Kit.

Credits

NASA/JPL-Caltech

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This image acquired on October 12, 2020 by NASAs Mars Reconnaissance Orbiter, shows an isolated, elongated mound (about 1 mile wide and 3.75 miles long) rising above the smooth, surrounding plains.
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This image acquired on October 12, 2020 by NASAs Mars Reconnaissance Orbiter, shows an isolated, elongated mound (about 1 mile wide and 3.75 miles long) rising above the smooth, surrounding plains.
A Technicolor Mound near Oxia Planum
Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from three different NASA Mars orbiters.
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Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from five instruments on three different NASA Mars orbiters, including physical properties from THEMIS (left) and mineral information from CRISM (right).
Multiple Instruments Used for Mars Carbon Estimate
NASA’s Perseverance rover took these zoomed-in images of a layered outcrop (just below center of   image) nicknamed “Artuby” on June 17, 2021 (the 116th sol, or Martian Day, of its mission), from a...
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NASA’s Perseverance rover took these zoomed-in images of a layered outcrop (just below center of image) nicknamed “Artuby” on June 17, 2021 (the 116th sol, or Martian Day, of its mission), from a little more than a third of a mile (615 meters) away.
SuperCam Image of 'Artuby'
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
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Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars
NASA's Mars Exploration Rover Opportunity has been on the western rim of Endeavour Crater in Meridiani Planum for about two years.
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NASA's Mars Exploration Rover Opportunity has been on the western rim of Endeavour Crater in Meridiani Planum for about two years.
Color View From Orbit Showing Opportunity in 'Botany Bay' (Unannotated)
Meet some of the women team members and hear about the exciting and challenging jobs they do in science and engineering while working with Mars rover Curiosity.
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Meet some of the women team members and hear about the exciting and challenging jobs they do in science and engineering while working with Mars rover Curiosity.
Women Working On Mars: Erisa Hines
Download a PDF of the Mars Sample Return Lithograph.
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Mars Sample Return lithograph
Mars Sample Return Lithograph
Drainage Near Crater in Terra Sabaea.
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Drainage Near Crater in Terra Sabaea.
Drainage Near Crater in Terra Sabaea
This stereo vista from NASA's Mars Exploration Rover Opportunity shows "Wdowiak Ridge," from left foreground to center, as part of a northward look with the rover's tracks visible at right. The ima...
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This stereo vista from NASA's Mars Exploration Rover Opportunity shows "Wdowiak Ridge," from left foreground to center, as part of a northward look with the rover's tracks visible at right.
Opportunity's Northward View of 'Wdowiak Ridge' (Stereo)
Mars's seasonal polar caps are composed primarily of carbon-dioxide frost.
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Mars's seasonal polar caps are composed primarily of carbon-dioxide frost.
Seasonal Processes-Omega Sublimation
Common to the northern plains of Mars are rock and boulder strewn landscapes otherwise devoid of major features except a few impact craters. This image in the Cydnus Rupes region of northern Utopia...
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Boulder Strewn Plain in Northern Utopia Planitia
Boulder Strewn Plain in Northern Utopia Planitia
This "ring trough" or eroded pit crater, is located in the rugged southern highland terrain known as Noachis Terra. The HiRISE image shows the layered, boulder-rich wall rock facing to the northeas...
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Geologically young gullies are a prime target for the HiRISE camera. Gullies are located in a variety of settings and are found all over Mars. This "ring trough" or eroded pit crater, is located in the rugged southern highland terrain known as Noachis Terra. The HiRISE image shows the layered, boulder-rich wall rock facing to the northeast and gullies that are transporting material downslope. The material collects into debris aprons along the walls, which often exhibit narrow channels along its surface.
Gullies on Southwest Slope of Ring Trough in Noachis Terra
Is frozen carbon dioxide a key to features in some Martian gullies? To find out, scientists grabbed a bag of dry ice and took a road trip.
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Dry Ice Moves on Mars
Dry Ice Moves on Mars
This inner slope of a Martian crater has several of the seasonal dark streaks called "recurrent slope lineae," or RSL, that a November 2017 report interprets as granular flows, rather than darkenin...
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Seasonal Dark Streaks in Tivat Crater, Mars
Seasonal Dark Streaks in Tivat Crater, Mars
This color-enhanced view shows the terrain around the rover's landing site within Gale Crater on Mars.
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This color-enhanced view shows the terrain around the rover's landing site within Gale Crater on Mars.
A Whole New World for Curiosity
A lunar eclipse, a solar eclipse and Mars has a close encounter with a comet.
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What's Up for October?
What's Up for October?
NASA's Mars 2020 spacecraft undergoes examination prior to an acoustic test in the Environmental Test Facility at NASA's Jet Propulsion Laboratory in Pasadena, California.
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NASA's Mars 2020 spacecraft undergoes examination prior to an acoustic test in the Environmental Test Facility at NASA's Jet Propulsion Laboratory in Pasadena, California.
Prepping Mars 2020 for Sound
The Mars Helicopter is a technology demonstration that will fly as a secondary payload with the Mars 2020 mission. It will demonstrate the potential of aerial flight on Mars, which may enable more ...
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The Mars Helicopter is a technology demonstration that will fly as a secondary payload with the Mars 2020 mission. It will demonstrate the potential of aerial flight on Mars, which may enable more ambitious missions in the future.
NASA Mars Helicopter Technology Demonstration
These dark streaks, also known as “slope streaks,” resulted from dust avalanches on Mars. The HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter captured them on Dec. 26, 2017.
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These dark streaks, also known as “slope streaks,” resulted from dust avalanches on Mars. The HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter captured them on Dec. 26, 2017.
HiRISE Spots Slope Streaks Fanning Out on Mars
In this image, taken on June 13, 2019, engineers at JPL install the starboard legs and wheels — otherwise known as the mobility suspension — on the Mars 2020 rover.
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In this image, taken on June 13, 2019, engineers at JPL install the starboard legs and wheels — otherwise known as the mobility suspension — on the Mars 2020 rover.
Mars 2020 Gets Its Wheels
Computer-generated visualization of the orbital paths (white dots) taken by the MAVEN spacecraft as it mapped winds (blue lines) in the Martian upper atmosphere.
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Computer-generated visualization of the orbital paths (white dots) taken by the MAVEN spacecraft as it mapped winds (blue lines) in the Martian upper atmosphere.
MAVEN Maps Wind in the Martian Upper Atmosphere
The Mars Color Imager (MARCI), shown here with a gloved hand for scale, is designed to produce a global map to help characterize daily, seasonal and year-to-year variations in Mars' climate, provid...
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The Mars Color Imager (MARCI), shown here with a gloved hand for scale, is designed to produce a global map to help characterize daily, seasonal and year-to-year variations in Mars' climate, providing a daily weather report for Mars.
Mars Color Imager (MARCI) for Mars Reconnaissance Orbiter
NASA’s Mars Reconnaissance Orbiter used its Context Camera to capture this image of Bosporos Planum, a location on Mars. The white specks are salt deposits found within a dry channel. The largest i...
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NASA’s Mars Reconnaissance Orbiter used its Context Camera to capture this image of Bosporos Planum, a location on Mars. The white specks are salt deposits found within a dry channel. The largest impact crater in the scene is nearly 1 mile (1.5 kilometers) across.
MRO's View of Salt Deposits in Bosporos Planum
Download a PDF of the Mars Sample Return sticker.
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Download a PDF of the Mars Sample Return sticker.
Mars Sample Return Sticker
NASA's Opportunity rover captured an image of this rock nicknamed "Jornada del Muerto" while in Perseverance Valley. The wind-carved streaks along its face were very similar to rocks seen at the ri...
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Close up of a Martian rock nicknamed "Jornada del Muerto"
Opportunity Discovers 'Dead Man's Journey'

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