Paramour Rupes

Red-cyan glasses will help you see the impressive heights of Paramour Rupes in this 3D view. Paramour is a large cliff (well over 600 meters high at places!) that formed when one block of crust was thrust forward over another, resulting in a feature known as a lobate scarp. Paramour Rupes is located to the southwest of the Caloris basin, and the small knobs that litter the scene are thought to be blocks of ejecta from the Caloris impact event. For ease of stereo viewing, this anaglyph has been rotated so that north is toward the left.

This image pair was acquired as a targeted set of stereo images. Targeted stereo observations are acquired at resolutions much higher than that of the 200-meter/pixel stereo base map. These targets acquired with the NAC enable the detailed topography of Mercury's surface to be determined for a local area of interest.

Date acquired: June 18, 2014
Image Mission Elapsed Time (MET): 45386688, 45387906
Image ID: 6520353, 6520362
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -4.99°
Center Longitude: 146.3°E
Resolution: 110 meters/pixel
Scale: This scene is approximately 110 km (68 miles) across
Incidence Angle: 63.8°
Emission Angle: 37.2°
Phase Angle: 97.7°

Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Sunrise Near the South Pole

Today's image features a large area near the south pole of Mercury. On the right side of this image, going from top to bottom are both the Terror Rupes and Eltanin Rupes. In the middle of the right edge is Alver, a peak-ring crater. Below Alver is Disney, a crater named after the animator Walt Disney.

Date acquired: June 16, 2014
Image Mission Elapsed Time (MET): 45232494, 45232490, 45232488
Image ID: 6510119, 6510117, 6510116
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filters: 9, 7, 6 (996, 748, 433 nanometers) in red, green, and blue
Center Latitude: -83.00°
Center Longitude: 40.17° E
Resolution: 2988 meters/pixel
Scale: This image is 1585 km (985 miles) across.
Center Incidence Angle: 85.3°
Center Emission Angle: 14.1°
Center Phase Angle: 99.4°

Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Terror Rupes

We have seen limb images of Mercury many times before, and they never fail to showcase the geological diversity (and splendor!) of the innermost planet. This time, something fills the scene with terror -- Terror Rupes, to be precise, the long, cliff-like landform visible at the center of the scene. Terror Rupes is one of Mercury's most prominent lobate scarps, and was named for HMS Terror, an eighteenth-century warship that later participated in scientific polar explorations. (For an explanation for how lobate scarps likely form, see this previous featured image.)

This image was acquired as part of MDIS's limb imaging campaign. Once per week, MDIS captures images of Mercury's limb, with an emphasis on imaging the southern hemisphere limb. These limb images provide information about Mercury's shape and complement measurements of topography made by the Mercury Laser Altimeter (MLA) of Mercury's northern hemisphere.

Date acquired: February 04, 2012
Image Mission Elapsed Time (MET): 236853865
Image ID: 1353252
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filter: 7 (748 nanometers)
Center Latitude: -69.3°
Center Longitude: 96.0° E
Resolution: 2.7 kilometers/pixel
Incidence Angle: 80.3°
Emission Angle: 50.9°
Phase Angle: 114.5°

Image credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Discovery Rupes at Rameau Crater

Although one of Mercury's largest lobate scarps, Discovery Rupes is by no means an unusual type of landform on the innermost planet. In fact, scarps cover the surface, and are interpreted to be the result of crustal shortening as Mercury's interior cooled and contracted. In this dramatic view of Discovery Rupes, taken with the Sun low in the sky, the relief along 400-km-long structure can be clearly seen as it cross-cuts Rameau crater.

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week.

Date acquired: September 23, 2013
Image Mission Elapsed Time (MET): 22261149
Image ID: 4875898
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -55.0°
Center Longitude: 322.2° E
Resolution: 246 meters/pixel
Scale: The field of view in this image is about 260 km (162 mi.) from top to bottom
Incidence Angle: 66.87°
Emission Angle: 39.74°
Phase Angle: 106.61°
North is to the top left of the image.

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Ride Along With Messenger (Video 1)

This movie was assembled from 284 individual NAC images. Most of the images were acquired four seconds apart, the fastest that MDIS is capable of taking full resolution images, but the movie is shown with 15 images per second. In the second half of the movie, Mirni Rupes can be seen in the top right.

These images were acquired as part of the NAC ride-along imaging campaign. When data volume is available and MDIS is not acquiring images for its other campaigns, high-resolution NAC images are obtained of the surface. These images are designed not to interfere with other instrument observations but take full advantage of periods during the mission when extra data volume is available.

Date acquired: October 04, 2013
Image Mission Elapsed Time (MET): 23235568-23236706
Image ID: 4945491-4945774
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Initial Center Latitude: -33.79°
Initial Center Longitude: 310.4° E
Final Center Latitude: -43.43°
Final Center Longitude: 324.6° E
Resolution: 145-174 meters/pixel
Scale: The first image is 148 kilometers (92 miles) across
Incidence Angle: 75.7°-87.7°
Emission Angle: 3.0°-15.2°
Phase Angle: 72.6°-72.5°

Video credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Possible Volcanic Vent Near Discovery Rupes

Different lighting conditions can reveal different insights into Mercury's surface. Check out this dramatic example of Discovery rupes. Today's image shows the same proposed volcanic vent that was featured last week, but this image was obtained with the Sun more nearly overhead. With this new view, you can see areas of the surface that were previously hidden in shadows.

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week.

Date acquired: June 06, 2013
Image Mission Elapsed Time (MET): 12831164
Image ID: 4206165
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 24.34°
Center Longitude: 148.3° E
Resolution: 28 meters/pixel
Scale: The diameter of the small crater to the left of the proposed vent is about 5 km (3 miles)
Incidence Angle: 26.7°
Emission Angle: 8.5°
Phase Angle: 35.2°

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Alvin Rupes

Lobate scarps are one of the most common types of landform on Mercury, and frequently cross-cut impact craters of all sizes. However, the example in this image, termed Alvin Rupes, is one of only a very small subset of scarps that are accompanied by thin, linear depressions on their upper surfaces. One possibility is that these features are graben -- fault-bounded troughs that form when rock is extended -- like those seen in Caloris basin, for example. If so, then these graben are among the only such structures known to occur outside of volcanically flooded impact basins and craters.

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week.

Date acquired: July 3, 2013
Image Mission Elapsed Time (MET): 15167012
Image ID: 4372157
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 7.8°
Center Longitude: 151.1° E
Resolution: 54 meters/pixel
Scale: The crater in the center of the image is about 12 km (7.5 mi.) across
Incidence Angle: 75.6°
Emission Angle: 12.6°
Phase Angle: 88.2°
North is up in this image.

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Rupes

Today's image features a scarp, or cliff face, which is longer than the 77 km shown in this frame. Scarps form as one block of crust is thrusted forward over another, which can result from the cooling of the planet's interior causing global contraction. On Mercury, scarps are called "rupes," which is Latin for cliff.

This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week.

Date acquired: July 08, 2013
Image Mission Elapsed Time (MET): 15627633
Image ID: 4404792
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 20.47°
Center Longitude: 141.0° E
Resolution: 51 meters/pixel
Scale: Image width is about 65 km (40.4 miles)
Incidence Angle: 83.4°
Emission Angle: 38.9°
Phase Angle: 45.4°

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Belgica Rupes

This image highlights the difference between the areas on and below the newly named Belgica Rupes. The arrows show Belgica's location, stretching along most of this image for about 764 km. Notice how some of the smaller, newer craters obscure the scarp line, while the older craters were clearly disrupted by the formation of Belgica Rupes.

The word 'rupes' comes from the latin word for cliff. All rupes on Mercury are named after vehicles of exploration. Belgica was a Belgian ship that explored the south pole of earth in 1898. Belgian Rupes is also very close to the southern pole of Mercury. It's name was approved by the IAU on June 6, 2013 along with 9 other rupes.

Date acquired: August 17, 2011
Image Mission Elapsed Time (MET): 222063126, 222063130, 222063122
Image ID: 642667, 642668, 642666
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filters: 3, 4, 6 (479, 558, 433 nanometers) in red, green, and blue
Center Latitude: -52.80°
Center Longitude: 64.08° E
Resolution: 896 meters/pixel
Scale: Belgica Rupes extends 764 km (475 miles).
Incidence Angle: 63.3°
Emission Angle: 0.4°
Phase Angle: 63.2°

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Waters Crater, et al

This WAC (Wide Angle Camera) image shows a large portion of the planet, known as a limb image. Prominent in this image is Waters crater in the top left corner, distinctive because of its bright rays and dark impact melt flow. Also identifiable in this picture are Beethoven basin, as well as the Bello crater, Rumi crater, Philoxenus crater, and partly visible: Palmer Rupes.

Date acquired: April 14, 2011
Image Mission Elapsed Time (MET): 211284337
Image ID: 130687
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filter: 7 (748 nanometers)
Center Latitude: -21.12°
Center Longitude: 249.8° E
Resolution: 884 meters/pixel
Scale: Mercury's diameter is 4880 kilometers (3030 miles).
Incidence Angle: 69.6°
Emission Angle: 63.7°
Phase Angle: 28.0°

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Ten Newly-Named Rupes

From the USGS Astrogeology Science Center:

The Working Group for Planetary System Nomenclature has approved new names for ten rupēs on Mercury: Alvin Rupes, Belgica Rupes, Calypso Rupes, Carnegie Rupes, Duyfken Rupes, Eltanin Rupes, Enterprise Rupes, Nautilus Rupes, Palmer Rupes, and Terror Rupes. For more information, see the Gazetteer of Planetary Nomenclature.

A Tribute to Messenger

This video showcases a small sampling of the thousands of images taken by the spacecraft, as well as animations illustrating how MESSENGER moves in orbit and how its orbit has changed during the mission.

The opening sequence is from the approach images from the first flyby in 2008. The first animation to follow (at 0:15) shows MESSENGER in its primary mission 12-hour orbit. The relevance of the November 9, 2011, date is that this was when the MESSENGER team was advised that NASA had approved the proposal for an extended mission, allowing the mission to continue making new observations from March 2012 to March 2013. The animation at 0:22 gives you an idea of the movement and gyrations ("dancing") that the spacecraft undergoes while it performs a schedule packed full of observations that take place over one Earth day. The animation sequence at 0:59 gives you a "top down" view over Mercury's north pole from when MESSENGER first went into orbit until several months into the extended mission. The apparent size of the orbit shrinks from the start of the animation to the end, as shortly into the extended mission, MESSENGER's orbital period was shrunk from 12-hours to 8-hours. The animation sequence at 1:44 shows MESSENGER's "dance" on the first day of the extended mission. The other images and embedded movies can be found in the Gallery section of the MESSENGER website.

Some highlight images of note include:

At 0:48 - Blue rays of Bek crater
At 0:54 - Basho crater
At 0:57 - Poe crater in Caloris basin
At 1:17 - MASCS instrument surface scans in ultraviolet and infrared
At 1:19 - A perspective view of the northern polar region, color-coded to MLA topography
At 1:27 - Rembrandt impact basin
At 1:29 - Rembrandt impact basin superimposed on the US for size comparison
At 1:34 - Rachmaninoff impact basin, 3D effect crated using the digital elevation model
At 1:34 - Debussy crater
At 1:58 - Beagle rupes
At 2:04 - Mosaic view of north pole, showing the shadowed regions
At 2:06 - As previous, with superimposed radar data indicating likely water-ice deposits
At 2:11 - A volcanic vent near the edge of Caloris basin
At 2:34 - Derain crater
At 2:36 - Disney crater and two unnamed craters that resemble Mickey Mouse
At 2:38 - Basho crater while the Sun is low in the sky
At 2:40 - Basho crater again, but now with the Sun nearly overhead
At 2:45 - Degas crater
At 2:58 - 'Weird terrain' at the Caloris antipode
At 3:03 - Waters crater with the 'blue tongue' of dark impact melt material
At 3:10 - Seuss crater
At 3:13 - Caloris basin
At 3:15 - Pit in Scarlatti crater, with prominent hollows on the pit rim
At 3:17 - Enhanced color of Caloris basin
At 3:22 - A lava channel that had flowed into the Kofi crater
At 3:29 - More detail of Caloris basin floor
At 3:30 - The young, bright-rayed Mena crater
At 3:37 - Central peaks of Eminescu crater, with hollows around the bases of the peaks
At 3:39 - Apollodorus and Pantheon fossae
At 3:41 - The hollows on the floor of Sander crater

The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MDIS acquired 88,746 images and extensive other data sets. MESSENGER is now in a year-long extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals.

Video credit: Images and animation stills courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington. Music: "Mercury Ridge" by Simon Wilkinson (thebluemask.com). Video creation and time-lapse animations by Mark 'Indy' Kochte.

Victoria Rupes

This image is a portion of the MDIS global mosaic basemap that was acquired during MESSENGER's first year in orbit. The scene, with north to the right, shows a geological feature termed Victoria Rupes -- a long cliff or scarp that formed when Mercury shrank slightly as its core cooled. Rupes on Mercury are named for ships of discovery, and Victoria Rupes is named for the Victoria that formed part of Ferdinand Magellan's fleet in his 1519-1522 effort to circumnavigate Earth.

This geologic feature is of particular interest to MESSENGER scientists because it is part of a larger, linear set of contractional structures that may correspond to what is termed a fold-and-thrust (FAT) belt on Earth. FAT belts are common terrestrial surface features, and form when the crust is shortened due to compressional tectonism. Identifying FAT belts on Mercury will help scientists understand in more detail how that planet's crust has deformed through time.

Date Created: February 10, 2012
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
Latitude Range: 47° N to 59° N
Longitude Range: 321° E to 331° E
Resolution: 250 meters/pixel
Scale: The crater just left of center is approximately 42 km (26 mi.) in diameter
Projection: Azimuthal equidistant

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Fram Rupes

One hundred years ago, on December 14, 1911, Norwegian explorer Roald Amundsen and his party became the first people to reach the Earth's south pole. The name of the ship that carried Amundsen to Antarctica was the Fram. The image above shows a portion of Fram Rupes on the planet Mercury, a long scarp (cliff) formed by compressive forces generated as the planet's interior cooled and contracted.

Date acquired: November 06, 2011
Image Mission Elapsed Time (MET): 229066087
Image ID: 978519
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: -55.5°
Center Longitude: 267.8° E
Resolution: 152 meters/pixel
Scale: The edges of the image are about 157 km long.
Incidence Angle: 67.2°
Emission Angle: 14.9°
Phase Angle: 81.2°

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Mercury Landscape

When MESSENGER first flew by Mercury on January 14, 2008, MDIS acquired images of a large portion of Mercury's surface that had never previously been seen by spacecraft. This mosaic of NAC images shows some of the geologic features discovered during that first flyby that have been subsequently named: the curving cliff face of Beagle Rupes, the elongated crater Sveinsdottir, and the craters Izquierdo and Kunisada flooded with lava.

This year, the MESSENGER spacecraft is positioned once again to visit the Solar System's innermost planet. However, this time, the spacecraft won't just pass by. On March 18, 2011, a 15-minute maneuver will place MESSENGER in orbit about Mercury, making it the first spacecraft ever to do so. The MESSENGER mission will then begin an extensive year-long science campaign to unravel Mercury's mysteries. 2011 promises to be an exciting year of further discoveries for the MESSENGER mission.

Date Acquired: January 14, 2008
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Scale: Izquierdo Crater is 170 kilometers (106 miles) in diameter.

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Long Scarp

Extending from the left edge of this image diagonally toward the lower right corner is a long scarp (cliff) face. This scarp runs through a large ancient crater in the center of the frame and was seen for the first time during MESSENGER's second Mercury flyby. Planetary geologists use the Latin term "rupes" for scarps on Mercury. Scarps such as this one have been identified all over the planet. The presence of many long and high scarps suggests a history for Mercury that is unlike that of any of the other planets in the Solar System. These giant scarps are believed to have formed when Mercury's interior cooled and the entire planet contracted slightly as a result, causing the surface rocks to fracture and some blocks of crust to thrust over others along great faults. Determining the geometry of such scarps on Mercury and information on the times that deformation occurred can thus be used to understand the thermal history of the planet. Next year, when the MESSENGER spacecraft is in orbit around Mercury, MDIS will acquire for the first time global imaging coverage of Mercury's surface with lighting conditions optimal for identifying such scarps.

Date Acquired: October 6, 2008
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Scale: The large crater crosscut by the scarp is approximately 110 kilometers (70 miles) in diameter.

Photo credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington