Difference between revisions of "LEND"

From The Moon
Jump to: navigation, search
Line 2: Line 2:
 
=Lunar Exploration Neutron Detector (LEND)=
 
=Lunar Exploration Neutron Detector (LEND)=
 
<div id="toc">
 
<div id="toc">
=Table of Contents=
+
[[Image:lend-instrument.jpg|lend-instrument.jpg]]<br /> '''Left:''' Credit: ''[http://www.nasa.gov/mission_pages/LRO/spacecraft/index.html NASA]'' - photo of ''LEND'' instrument. <br /> <br />  
<div style="margin-left: 1em">[#Lunar Exploration Neutron Detector (LEND) Lunar Exploration Neutron Detector (LEND)]</div><div style="margin-left: 2em">[#Lunar Exploration Neutron Detector (LEND)-Description Description]</div><div style="margin-left: 2em">[#Lunar Exploration Neutron Detector (LEND)-Description: Wikipedia Description: Wikipedia]</div><div style="margin-left: 2em">[#Lunar Exploration Neutron Detector (LEND)-Additional Information Additional Information]</div><div style="margin-left: 2em">[#Lunar Exploration Neutron Detector (LEND)-LPOD Articles LPOD Articles]</div><div style="margin-left: 2em">[#Lunar Exploration Neutron Detector (LEND)-Bibliography Bibliography]</div></div>[[Image:lend-instrument.jpg|lend-instrument.jpg]]<br /> '''Left:''' Credit: ''[http://www.nasa.gov/mission_pages/LRO/spacecraft/index.html NASA]'' - photo of ''LEND'' instrument. <br /> <br />  
 
 
==Description==
 
==Description==
 
  The LEND instrument is a payload onboard the [[LRO|Lunar Reconnaissance Orbiter]] spacecraft that launched to the Moon on 19 June 2009. Consisting of nine detectors to measure fluxes of thermal, epithermal, and fast neutrons (produced from continuous cosmic ray bombardment of the lunar surface), LEND has the ability to detect water-ice deposits in Permanently Shadowed Regions (PSRs) at both lunar poles, and map hydrogen distribution (~ 100 ppm) in the shallow subsurface down to a resolution of 5 km. The Russian-made instrument is the first collimated neutron instrument to ever fly in space. <br /> <br />  
 
  The LEND instrument is a payload onboard the [[LRO|Lunar Reconnaissance Orbiter]] spacecraft that launched to the Moon on 19 June 2009. Consisting of nine detectors to measure fluxes of thermal, epithermal, and fast neutrons (produced from continuous cosmic ray bombardment of the lunar surface), LEND has the ability to detect water-ice deposits in Permanently Shadowed Regions (PSRs) at both lunar poles, and map hydrogen distribution (~ 100 ppm) in the shallow subsurface down to a resolution of 5 km. The Russian-made instrument is the first collimated neutron instrument to ever fly in space. <br /> <br />  
Line 21: Line 20:
 
<br />
 
<br />
 
----
 
----
<br />  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>
+
<br />  </div>

Revision as of 16:30, 15 April 2018

Lunar Exploration Neutron Detector (LEND)

lend-instrument.jpg
Left: Credit: NASA - photo of LEND instrument.

Description

The LEND instrument is a payload onboard the Lunar Reconnaissance Orbiter spacecraft that launched to the Moon on 19 June 2009. Consisting of nine detectors to measure fluxes of thermal, epithermal, and fast neutrons (produced from continuous cosmic ray bombardment of the lunar surface), LEND has the ability to detect water-ice deposits in Permanently Shadowed Regions (PSRs) at both lunar poles, and map hydrogen distribution (~ 100 ppm) in the shallow subsurface down to a resolution of 5 km. The Russian-made instrument is the first collimated neutron instrument to ever fly in space. 

Description: Wikipedia


Additional Information

  • Recent LEND (2010):
    lend-maps-small.jpg
    Images above show just two map-views from recent LEND data as reported by Anton Sanin (et al) in last September's LEAG Meeting (2010). The maps are of the count rate of epithermal neutrons (neutrons having an energy in the range immediately above the thermal range, roughly between 0.02 and 100 electronvolts) at both the North and South lunar poles (above 80 degrees latitude). Blue areas represent Neutron Supressed Regions (NSRs) due to detection of increased Hydrogen signatures (of water-ice deposits?), while the gray and black colour contours represent surface relief and permanently shadowed regions. As of writing (24 Oct., 2010), while the above-mentioned areas found by LEND confirm those neutron suppression spots as discovered by the Lunar Prospector mission back in 1998/99, the findings also have thrown light on relationships between individual PSRs and NSRs. For example: some PSR areas correlate very well with NSRs; other PSRs correlate in part (only) with NSRs that extend well beyond the shadowed regions; however, there are some PSRs that don't correlate at all with detected NSRs. Images credit NASA. Click for larger view.- JohnMoore2 JohnMoore2


LPOD Articles


Bibliography