Lunar Rotation and Flyby from Clementine Data

  • Released Friday, June 9, 1995
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Clementine was a joint project between the Strategic Defense Initiative Organization and NASA. The objective of the mission was to test sensors and spacecraft components under extended exposure to the space environment and to make scientific observations of the Moon and the near-Earth asteroid 1620 Geographos. Clementine was launched on 25 January 1994 at 16:34 UTC (12:34 PM EDT) from Vandenberg AFB aboard a Titan II G rocket. After two Earth flybys, lunar insertion was achieved on February 21. Lunar mapping took place over approximately two months, in two parts. The first part consisted of a 5 hour elliptical polar orbit with a perilune of about 400 km at 28 degrees S latitude. After one month of mapping the orbit was rotated to a perilune of 29 degrees N latitude, where it remained for one more month. This allowed global imaging as well as altimetry coverage from 60 degrees S to 60 degrees N.

Video slate image reads "Lunar Topography from the Clementine Mission".

Video slate image reads "Lunar Topography from the Clementine Mission".

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Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

Release date

This page was originally published on Friday, June 9, 1995.
This page was last updated on Wednesday, May 3, 2023 at 2:00 PM EDT.


Missions

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Series

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Papers used in this visualization

Maria T. Zuber, David E. Smith, Frank G. Lemoine, Gregory A. Neumann, The Shape and Internal Structure of the Moon from the Clementine Mission, Science, 16 December 1994, pp. 1839-1843.


Datasets used in this visualization

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