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In this movie, MESSENGER team members recount some highlights of the mission, originally planned to orbit Mercury for only one year, but ultimately orbiting the planet for more than four years. This movie was released on August 3, 2015, the 11th anniversary of the launch of the MESSENGER spacecraft.

This movie shows the total lunar eclipse of October 8, 2014, as viewed by MESSENGER. From Mercury, the Earth and Moon normally appear as if they were two very bright stars. During a lunar eclipse, the Moon seems to disappear during its passage through the Earth's shadow. This movie was constructed from 31 images taken two minutes apart, from 9:18 UTC to 10:18 UTC. The images start just before the Moon entered the darkest part of the Earth's shadow (the umbra).

This movie demonstrates a MASCS VIRS raster scan. The target is Lermontov crater in Mercury's mid latitudes, for which 258 spectra were consecutively taken 1 to 5 seconds apart. Each spectrum (green) is compared to Mercury's mean spectrum (black) between wavelengths of 300nm and 1450nm.

The MESSENGER Flyover Movie consists of 214 images acquired by the spacecraft's Narrow Angle Camera (NAC) on June 8, 2014. The NAC field of view looks toward the horizon along the direction of spacecraft motion as the probe crossed the terminator into night. MESSENGER flew over Mercury's north polar region, providing views of the planet's cratered terrain. Information in the available captioned version includes image acquisition time, local solar time, image location, spacecraft altitude, and image resolution. Broadcast-ready versions are also available. For additional details of what this movie illustrates, visit this aerial view and this higher-resolution mosaic of MESSENGER's flight path.

This movie was assembled from 284 individual NAC images acquired on 4 October, 2013. Most of the images were acquired 4 seconds apart, the fastest that MDIS was capable of taking full resolution images, but this 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.

This movie was assembled from 289 individual NAC images acquired on 4 October, 2013. Most of the images were acquired 4 seconds apart, the fastest that MDIS was capable of taking full resolution images, but this movie is shown with 15 images per second. The movie begins centered on the 191-km diameter Schubert basin. These images were acquired as part of the NAC ride-along imaging campaign.

This movie shows Mercury's globe as it rotates. A global color map of Mercury's surface has been created by mosaicking thousands of sets of images obtained by the MESSENGER Wide Angle Camera (WAC). The colors shown here are related to real variations in the spectral reflectance across the planet. This view captures both compositional differences and differences in how long materials have been exposed at Mercury's surface. Young crater rays, arrayed radially around fresh impact craters, appear light blue or white. Medium- and dark-blue areas are a geologic unit of Mercury's crust known as the "low-reflectance material," thought to be rich in a dark, opaque mineral. Tan areas are plains formed by eruption of highly fluid lavas. The color base map shown here consists of MDIS images taken through eight different color filters. It is part of a global color map that covers more than 99% of Mercury's surface with an average resolution of about 1 kilometer per pixel.

This is a movie of Mercury's Rachmaninoff impact basin. An enhanced-color image has been draped over a digital elevation model of the surface. The vertical exaggeration is 7 times. The basin's outer rim is about 306 km in diameter and the inner (peak) ring is about 140 km in diameter. The volcanic smooth plains within the center appear tan in this presentation, emphasizing their compositional contrast with the dark, bluer rocks that form the peak ring mountains. Images from the Mercury Dual Imaging System on board NASA's MESSENGER spacecraft were processed to provide the color and elevation information used to create this view.

This animation displays the illumination of the topography of Mercury's north polar region, showing the small proportion of sunlight that reaches the Prokofiev crater floor and rim. The north-facing portions of the rim and interior remain in perpetual shadow, as do those of numerous other craters. The movie simulates approximately one half of a Mercury solar day (176 Earth days) and uses the digital terrain model derived from MLA measurements. Contrast has been enhanced for television display.

This movie shows 89 wide-angle camera (WAC) images of Mercury's south polar region acquired by the Mercury Dual Imaging System (MDIS) over one complete Mercury solar day (176 Earth days) in 2011. This dataset enabled the illumination conditions at Mercury's south polar region to be quantified and the identification of areas of permanent shadow. Each image is shown in polar stereographic projection, extending northward to 73° S, and 0° longitude is at the top. The large crater near Mercury's south pole, Chao Meng-Fu, has a diameter of 180 km.

Watch a movie that shows the locations at which energetic electrons were detected by MESSENGER between March 24 and June 3, 2011. In the coordinate system used (known as the Mercury solar orbital, or MSO, coordinates), the Sun is always in a fixed direction (here +X-axis). The events are well distributed in local time, but most are seen when the spacecraft is in the northern hemisphere. MESSENGER's X-ray Spectrometer (XRS) responds to electrons initially with lower energies but in a manner analogous to the GRS.

Watch a movie that shows the location of Mercury's magnetic equator determined on successive orbits as the point where the direction of the internal magnetic field is parallel to the spin axis of the planet. This magnetic equator is well north of the planet's geographic equator (indicated by the horizontal gray line). The best-fitting internal dipole magnetic field is located about 0.2 Mercury radii, or 480 km, northward of the planet's center.

Watch a movie that shows the MLA profiles acquired between 29 March and 24 May. Elevation along track (relative to a sphere of radius 2,440 km) is shown by the color scale. Note the broad area of generally low elevations in Mercury's north polar region. The total range in elevation measured by MLA to date is more than 9 km. Orthographic projection centered on the north pole; the outmost circle corresponds to Mercury's equator.

Watch a movie that shows the current monochrome imaging coverage as of June 16, 2011, centered at 240° E, and zooms in to highlight one of the many striking features seen during the first few months of orbital operations. At 9.0° S, 254.7° E, impact melt flowed from an unnamed, 13-km-diameter impact crater, extending outward more than one crater diameter from the rim.

As MESSENGER completed its successful flyby of Mercury, the Narrow Angle Camera (NAC), part of the Mercury Dual Imaging System (MDIS), took images of the planet as the spacecraft departed. Beginning on January 14, 2008, about 100 minutes after MESSENGER's closest pass by the surface of Mercury, until January 15, 2008, about 19 hours later, the NAC acquired one image every four minutes. In total, 288 images were snapped during this time and were compiled sequentially to produce this movie. At the start of the movie, MESSENGER is about 34,000 kilometers (about 21,000 miles) from Mercury, and the first image has a field of view of about 950 kilometers (about 590 miles) in width. At the end of the movie, the MESSENGER spacecraft is a distance of about 440,000 kilometers (270,000 miles) from Mercury.

This movie shows the end of MESSENGER's first encounter with Mercury. MESSENGER flew by Mercury two additional times during the mission, in October 2008 and September 2009. In March 2011, MESSENGER entered into an orbit around Mercury and began a year-long scientific investigation of the planet.

On January 13, 2008, beginning 30 hours before MESSENGER's closest approach to Mercury, the Wide Angle Camera, part of the Mercury Dual Imaging System (MDIS), began snapping images as it approached the planet. Over this period, MESSENGER imaged the planet once every 20 minutes to produce this approach sequence, which has been compiled into a movie. At the start of the movie, the MESSENGER spacecraft is about 630,000 kilometers (about 390,000 miles) from Mercury. The movie ends when MESSENGER is about 34,000 kilometers (about 21,000 miles) from Mercury and about 100 minutes before its closest approach, when it passed a mere 200 kilometers (124 miles) above Mercury's surface.

In the approach movie, Mercury appears as a sunlit crescent. During the encounter, MESSENGER passed over the night side of the planet, experienced its closest approach with Mercury, and then emerged into daylight. This encounter was the first of three flybys of Mercury for the MESSENGER mission.

Between January 9 and 13, 2008, as the MESSENGER probe approached Mercury for its first flyby, the Narrow Angle Camera, part of the Mercury Dual Imaging System (MDIS), acquired a series of images of the planet in support of spacecraft navigation. These images have been put together as frames in a movie. The final frame of the movie has the highest spatial resolution (20 km/pixel, 12 miles/pixel) and was recorded when the spacecraft was at a distance of about 760,000 kilometers (470,000 miles) from Mercury. Mercury is about 4880 kilometers (about 3030 miles) in diameter.

The Mercury-bound MESSENGER spacecraft captured several stunning images of Earth during a gravity assist swingby of its home planet on Aug. 2, 2005. Several hundred images, taken with the wide-angle camera in MESSENGER's Mercury Dual Imaging System (MDIS), were sequenced into a movie documenting the view from MESSENGER as it departed Earth. 2b1af7f3a8

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