LRO at the June 15, 2011 Lunar Eclipse: View from the Moon
For Lunar Reconnaissance Orbiter (LRO), the lunar eclipse on June 15, 2011 is likely to be the longest and darkest of its life. This matters because LRO relies on sunlight to power its systems and instruments. Although it spends half of every orbit on the night side of the Moon, each night side pass lasts only an hour. For the June 15 eclipse, LRO will be in the dark for more than twice as long.
During a previous total eclipse, LRO hibernated, turning off all of its instruments to conserve its battery power until the Moon emerged from the Earth's shadow. For the June 15 event, LRO will leave on the Diviner Lunar Radiometry Experiment. Diviner will measure the cooling of the Moon's surface during the eclipse. This unique temperature record is expected to reveal information about the roughness and composition of the swath of lunar surface visible to Diviner's sensors during the eclipse.
The visualization archived on this page shows the view of the eclipse from the Moon, looking back toward the Earth and the Sun. On the Moon, this event is a solar eclipse. As the Sun disappears behind the Earth, the umbral shadow sweeps across the lunar landscape, and as our eyes adjust to the darkness, the stars come out, and the lunar surface looks a dull red. The atmosphere of the Earth lights up as a red ring around the planet, the sunrises and sunsets all around the edge of the globe lending their faint light to the Moon while the Sun is otherwise blocked. At the start of the eclipse, Australia is facing us, but over time, the Moon sets in eastern Australia while southern Africa rotates into view. LRO streaks through the frame several times on its orbit 50 kilometers above the Moon's surface.
Other visualizations in this series depict the view of the eclipse
- along the shadow line, with the figures of the umbra, penumbra, and lunar and solar paths
- through a telescope on Earth
- flying above LRO as Diviner takes temperature measurements
A narrated piece that uses these visualizations is available in entry #10794. For an explanation of lunar eclipses, visit entry #10787.
The eclipse as viewed from the Moon.
The image layer containing the Moon, Earth, and Sun, with alpha channel.
The image layer containing the star field. The clump of stars in the upper left is M35, an open cluster in the constellation Gemini.
Alpha channel for the clock overlay.
Print resolution still. Looking from the Moon's dark side toward the Sun, the limb of the Moon is visible as the Sun begins to slip behind the Earth.
Print resolution still. The landscape of the Moon, foreground, is reddened by sunlight filtered through Earth's atmosphere. The Sun is obscured by the Earth, but the glow of its corona is visible. The Moon is setting in eastern Australia and rising in southern Africa. LRO flies through the frame.
Print resolution still. The landscape of the Moon, foreground, is reddened by sunlight filtered through Earth's atmosphere. The Sun is obscured by the Earth, but the glow of its corona is visible. The Moon is setting in eastern Australia and rising in southern Africa.
Print resolution still. The Moon, foreground, has left the Earth's umbra as the Sun emerges from behind the Earth. The Moon is highest in the sky for southern Africa.
Print resolution still. The Moon, foreground, has left the Earth's umbra as the Sun emerges from behind the Earth. The Moon is highest in the sky for southern Africa. LRO flies through the frame.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio
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Animator
- Ernie Wright (USRA)
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Producers
- Genna Duberstein (USRA)
- Chris Smith (HTSI)
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Scientist
- Richard Vondrak (NASA/GSFC)
Release date
This page was originally published on Wednesday, June 29, 2011.
This page was last updated on Wednesday, May 3, 2023 at 1:53 PM EDT.
Missions
This page is related to the following missions:Series
This page can be found in the following series:Datasets used
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Earth at Night [DMSP: OLS]
ID: 286 -
DEM (Digital Elevation Map) [LRO: LOLA]
ID: 653
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.