Difference between revisions of "LOLA"

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'''Left:''' Credit: ''[http://lunar.gsfc.nasa.gov/lola.html NASA]'' - photo of ''LOLA'' instrument. <br /> '''Right:''' Credit: [http://lunar.gsfc.nasa.gov/lola/images/smith_lola_ssr09.pdf David Smith] ''et al'' - another view.<br /> <div id="toc">
 
'''Left:''' Credit: ''[http://lunar.gsfc.nasa.gov/lola.html NASA]'' - photo of ''LOLA'' instrument. <br /> '''Right:''' Credit: [http://lunar.gsfc.nasa.gov/lola/images/smith_lola_ssr09.pdf David Smith] ''et al'' - another view.<br /> <div id="toc">
=Table of Contents=
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<br />  
<div style="margin-left: 1em">[#Lunar Orbiter Laser Altimeter (LOLA) Lunar Orbiter Laser Altimeter (LOLA)]</div><div style="margin-left: 2em">[#Lunar Orbiter Laser Altimeter (LOLA)-Description Description]</div><div style="margin-left: 2em">[#Lunar Orbiter Laser Altimeter (LOLA)-Description: Wikipedia Description: Wikipedia]</div><div style="margin-left: 2em">[#Lunar Orbiter Laser Altimeter (LOLA)-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Lunar Orbiter Laser Altimeter (LOLA)-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Lunar Orbiter Laser Altimeter (LOLA)-Bibliography Bibliography]</div></div><br />  
 
 
==Description==
 
==Description==
 
  The LOLA instrument is a payload onboard the [[LRO|Lunar Reconnaissance Orbiter]] spacecraft that launched to the Moon on 19 June 2009. Using five laser beams that illuminate the lunar surface (created from a single laser beam passing through a diffractive optical system), LOLA turns the reflected beams into data about the Moon. These data can include findings, for example, about the moon’s surface topography, its roughness, slope and reflectance, but also, primarily, provide vital information for a global geodetic [http://imbrium.mit.edu/DATA/LOLA_GDR/ grid] for the Moon.<br /> <br />  
 
  The LOLA instrument is a payload onboard the [[LRO|Lunar Reconnaissance Orbiter]] spacecraft that launched to the Moon on 19 June 2009. Using five laser beams that illuminate the lunar surface (created from a single laser beam passing through a diffractive optical system), LOLA turns the reflected beams into data about the Moon. These data can include findings, for example, about the moon’s surface topography, its roughness, slope and reflectance, but also, primarily, provide vital information for a global geodetic [http://imbrium.mit.edu/DATA/LOLA_GDR/ grid] for the Moon.<br /> <br />  
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<br />  
 
<br />  
 
==Additional Information==
 
==Additional Information==
* Recent LOLA data (2010):<br /> [http://the-moon.us/wiki/file/detail/Lola-nearside.jpg [[Image:Lola-nearside-small.jpg|Lola-nearside-small.jpg]]][http://the-moon.us/wiki/file/detail/Lola-eastside.jpg [[Image:Lola-eastside-small.jpg|Lola-eastside-small.jpg]]]<br />  Images above show just two views from recent LOLA research by [http://www.sciencemag.org/cgi/content/short/329/5998/1504 James Head] (''et al'') who carried out a global census of 5185 craters greater than or equal to 20 kilometres in size. Colours in ''Green'' represent the global ‘mean’ elevation value, ''Blue'' is below this value, while ''Yellow'' is above. Note, how the basin regions (dark regions) show less craters in the range, while those in the highland regions are much higher. Head’s research points to the fact that there were two populations of impactors in the early solar system history, and that the transition occurred near the time of the [[Mare%20Orientale|Orientale Basin]] event - around the [[Stratigraphy|Late Imbrium]] period (~ 3.85 to 3.75 bn years). <span class="membersnap">- [http://www.wikispaces.com/user/view/JohnMoore2 [[Image:JohnMoore2-lg.jpg|16px|JohnMoore2]]] [http://www.wikispaces.com/user/view/JohnMoore2 JohnMoore2]</span><br />  Credit: NASA’s ''[http://svs.gsfc.nasa.gov/vis/a000000/a003600/a003662/index.html Scientific Visualization Studio]''.
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* Recent LOLA data (2010):<br /> [http://the-moon.us/wiki/file/detail/Lola-nearside.jpg [[Image:Lola-nearside-small.jpg|Lola-nearside-small.jpg]]][http://the-moon.us/wiki/file/detail/Lola-eastside.jpg [[Image:Lola-eastside-small.jpg|Lola-eastside-small.jpg]]]<br />  Images above show just two views from recent LOLA research by [http://www.sciencemag.org/cgi/content/short/329/5998/1504 James Head] (''et al'') who carried out a global census of 5185 craters greater than or equal to 20 kilometres in size. Colours in ''Green'' represent the global ‘mean’ elevation value, ''Blue'' is below this value, while ''Yellow'' is above. Note, how the basin regions (dark regions) show less craters in the range, while those in the highland regions are much higher. Head’s research points to the fact that there were two populations of impactors in the early solar system history, and that the transition occurred near the time of the [[Mare%20Orientale|Orientale Basin]] event - around the [[Stratigraphy|Late Imbrium]] period (~ 3.85 to 3.75 bn years). <span class="membersnap">- JohnMoore2</span><br />  Credit: NASA’s ''[http://svs.gsfc.nasa.gov/vis/a000000/a003600/a003662/index.html Scientific Visualization Studio]''.
 
* LOLA’s laser pulses can be upto 140/sec working at approximately ±10 cm range measurements at 28 Hz.
 
* LOLA’s laser pulses can be upto 140/sec working at approximately ±10 cm range measurements at 28 Hz.
 
* Principal investigators: David Smith, Maria Zuber.
 
* Principal investigators: David Smith, Maria Zuber.
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  Head, J. W. ''et al'' (2010). [http://www.sciencemag.org/cgi/content/short/329/5998/1504 Global Distribution of Large Lunar Craters: Implications for Resurfacing and Impactor Populations] – Science, Vol. 329. no. 5998, pp. 1504 – 1507, 17 September 2010.<br />  Beatty, K. (2010). [http://www.skyandtelescope.com/news/103129789.html The Moon Through LRO’s Eyes] – ''Sky & Telescope'', September 2010.<br />  Smith, D. E. ''et al'' (2008). [http://lunar.gsfc.nasa.gov/lola/images/smith_lola_ssr09.pdf The Lunar Orbiter Laser Altimeter Investigation on the Lunar Reconnaissance Orbiter Mission] – ''Space Science Reviews'' 2008.<br /> <br />
 
  Head, J. W. ''et al'' (2010). [http://www.sciencemag.org/cgi/content/short/329/5998/1504 Global Distribution of Large Lunar Craters: Implications for Resurfacing and Impactor Populations] – Science, Vol. 329. no. 5998, pp. 1504 – 1507, 17 September 2010.<br />  Beatty, K. (2010). [http://www.skyandtelescope.com/news/103129789.html The Moon Through LRO’s Eyes] – ''Sky & Telescope'', September 2010.<br />  Smith, D. E. ''et al'' (2008). [http://lunar.gsfc.nasa.gov/lola/images/smith_lola_ssr09.pdf The Lunar Orbiter Laser Altimeter Investigation on the Lunar Reconnaissance Orbiter Mission] – ''Space Science Reviews'' 2008.<br /> <br />
 
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  This page has been edited 1 times. The last modification was made by <span class="membersnap">- [http://www.wikispaces.com/user/view/tychocrater [[Image:tychocrater-lg.jpg|16px|tychocrater]]] [http://www.wikispaces.com/user/view/tychocrater tychocrater]</span> on Jun 13, 2009 3:24 pm - ''afx3u2''siondate} - ''afx3u2''ondate} - ''afx3u2''</div>
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Latest revision as of 21:21, 16 April 2018

Lunar Orbiter Laser Altimeter (LOLA)

lola-instrument.jpg

lola-instrument2.jpg

Left: Credit: NASA - photo of LOLA instrument.
Right: Credit: David Smith et al - another view.


Description

The LOLA instrument is a payload onboard the Lunar Reconnaissance Orbiter spacecraft that launched to the Moon on 19 June 2009. Using five laser beams that illuminate the lunar surface (created from a single laser beam passing through a diffractive optical system), LOLA turns the reflected beams into data about the Moon. These data can include findings, for example, about the moon’s surface topography, its roughness, slope and reflectance, but also, primarily, provide vital information for a global geodetic grid for the Moon.

Description: Wikipedia


Additional Information

  • Recent LOLA data (2010):
    Lola-nearside-small.jpgLola-eastside-small.jpg
    Images above show just two views from recent LOLA research by James Head (et al) who carried out a global census of 5185 craters greater than or equal to 20 kilometres in size. Colours in Green represent the global ‘mean’ elevation value, Blue is below this value, while Yellow is above. Note, how the basin regions (dark regions) show less craters in the range, while those in the highland regions are much higher. Head’s research points to the fact that there were two populations of impactors in the early solar system history, and that the transition occurred near the time of the Orientale Basin event - around the Late Imbrium period (~ 3.85 to 3.75 bn years). - JohnMoore2
    Credit: NASA’s Scientific Visualization Studio.
  • LOLA’s laser pulses can be upto 140/sec working at approximately ±10 cm range measurements at 28 Hz.
  • Principal investigators: David Smith, Maria Zuber.
  • LOLA data are available to the public through the periodic releases of LRO datasets on NASA's PDS, and also sometimes a bit in advance on the MIT site.


LPOD Articles


Bibliography

Head, J. W. et al (2010). Global Distribution of Large Lunar Craters: Implications for Resurfacing and Impactor Populations – Science, Vol. 329. no. 5998, pp. 1504 – 1507, 17 September 2010.
Beatty, K. (2010). The Moon Through LRO’s EyesSky & Telescope, September 2010.
Smith, D. E. et al (2008). The Lunar Orbiter Laser Altimeter Investigation on the Lunar Reconnaissance Orbiter MissionSpace Science Reviews 2008.