NASA's Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on Feb. 23, 2025 — sol 4462, or Martian day 4,462 of the Mars Science Laboratory mission — at 21:43:37 UTC.
Does the USGS produce mapping for other planetary bodies?
The USGS Astrogeology Science Center was founded in 1963 to map the Moon and assist in training the Apollo astronauts. Currently its mission includes producing planetary maps and cartographic products which reveal topography, geology, topology, image mosaics and more, all made available to the international scientific community and the general public as a national resource.
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Is it true that Earth's magnetic field occasionally reverses its polarity? Is it true that Earth's magnetic field occasionally reverses its polarity?
What is a magnetic storm? What is a magnetic storm?
Do animals use the magnetic field for orientation? Do animals use the magnetic field for orientation?
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NASA's Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on Feb. 23, 2025 — sol 4462, or Martian day 4,462 of the Mars Science Laboratory mission — at 21:43:37 UTC.
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds.
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds.
by Ken Herkenhoff, USGS Astrogeology Science Center
by Ken Herkenhoff, USGS Astrogeology Science Center

USGS SIM 2888: Geologic map of the northern plains of Mars
By K. L. Tanaka, J. A. Skinner, and T. M. Hare
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/sim2888
USGS SIM 2888: Geologic map of the northern plains of Mars
By K. L. Tanaka, J. A. Skinner, and T. M. Hare
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/sim2888
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98% of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km.
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98% of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km.
This image shows two views of the trailing hemisphere of Jupiter's ice-covered satellite, Europa. The left image shows the approximate natural color appearance of Europa. The image on the right is a false-color composite version combining violet, green and infrared images to enhance color differences in the predominantly water-ice crust of Europa.
This image shows two views of the trailing hemisphere of Jupiter's ice-covered satellite, Europa. The left image shows the approximate natural color appearance of Europa. The image on the right is a false-color composite version combining violet, green and infrared images to enhance color differences in the predominantly water-ice crust of Europa.

Inset of USGS IMAP 1658: Geologic map of the Discovery Quadrangle of Mercury
By N. J. Trask and D. Dzurisin
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1658
Inset of USGS IMAP 1658: Geologic map of the Discovery Quadrangle of Mercury
By N. J. Trask and D. Dzurisin
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1658

USGS IMAP 1162: Geologic map of the south side of the Moon
By D.E. Wilhelms, K.A. Howard, and H. G. Wilshire
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1162
USGS IMAP 1162: Geologic map of the south side of the Moon
By D.E. Wilhelms, K.A. Howard, and H. G. Wilshire
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1162
1969 Earth Rise from Moon Apollo 11 - EROS History Project
1969 Earth Rise from Moon Apollo 11 - EROS History Project

USGS IMAP 515: (LAC-58) Geologic map of the Copernicus quadrangle of the moon
By H. H. Schmitt, N. J. Trask, and E. M. Shoemaker
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i515
USGS IMAP 515: (LAC-58) Geologic map of the Copernicus quadrangle of the moon
By H. H. Schmitt, N. J. Trask, and E. M. Shoemaker
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i515
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Related
How can I tell if I have found an impact crater? How can I tell if I have found an impact crater?
Is it true that Earth's magnetic field occasionally reverses its polarity? Is it true that Earth's magnetic field occasionally reverses its polarity?
What is a magnetic storm? What is a magnetic storm?
Do animals use the magnetic field for orientation? Do animals use the magnetic field for orientation?
What are the hazards of magnetic storms? What are the hazards of magnetic storms?
NASA's Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on Feb. 23, 2025 — sol 4462, or Martian day 4,462 of the Mars Science Laboratory mission — at 21:43:37 UTC.
NASA's Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on Feb. 23, 2025 — sol 4462, or Martian day 4,462 of the Mars Science Laboratory mission — at 21:43:37 UTC.
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds.
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Pluto on July 14, 2015. The image combines blue, red and infrared images taken by the Ralph/Multispectral Visual Imaging Camera (MVIC). Pluto's surface sports a remarkable range of subtle colors, enhanced in this view to a rainbow of pale blues, yellows, oranges, and deep reds.
by Ken Herkenhoff, USGS Astrogeology Science Center
by Ken Herkenhoff, USGS Astrogeology Science Center

USGS SIM 2888: Geologic map of the northern plains of Mars
By K. L. Tanaka, J. A. Skinner, and T. M. Hare
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/sim2888
USGS SIM 2888: Geologic map of the northern plains of Mars
By K. L. Tanaka, J. A. Skinner, and T. M. Hare
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/sim2888
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98% of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km.
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered at 180 degrees east longitude. The Magellan spacecraft imaged more than 98% of Venus at a resolution of about 100 meters; the effective resolution of this image is about 3 km.
This image shows two views of the trailing hemisphere of Jupiter's ice-covered satellite, Europa. The left image shows the approximate natural color appearance of Europa. The image on the right is a false-color composite version combining violet, green and infrared images to enhance color differences in the predominantly water-ice crust of Europa.
This image shows two views of the trailing hemisphere of Jupiter's ice-covered satellite, Europa. The left image shows the approximate natural color appearance of Europa. The image on the right is a false-color composite version combining violet, green and infrared images to enhance color differences in the predominantly water-ice crust of Europa.

Inset of USGS IMAP 1658: Geologic map of the Discovery Quadrangle of Mercury
By N. J. Trask and D. Dzurisin
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1658
Inset of USGS IMAP 1658: Geologic map of the Discovery Quadrangle of Mercury
By N. J. Trask and D. Dzurisin
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1658

USGS IMAP 1162: Geologic map of the south side of the Moon
By D.E. Wilhelms, K.A. Howard, and H. G. Wilshire
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1162
USGS IMAP 1162: Geologic map of the south side of the Moon
By D.E. Wilhelms, K.A. Howard, and H. G. Wilshire
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i1162
1969 Earth Rise from Moon Apollo 11 - EROS History Project
1969 Earth Rise from Moon Apollo 11 - EROS History Project

USGS IMAP 515: (LAC-58) Geologic map of the Copernicus quadrangle of the moon
By H. H. Schmitt, N. J. Trask, and E. M. Shoemaker
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i515
USGS IMAP 515: (LAC-58) Geologic map of the Copernicus quadrangle of the moon
By H. H. Schmitt, N. J. Trask, and E. M. Shoemaker
Map and associated documents available from the USGS Publications Warehouse: https://doi.org/10.3133/i515