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Latest revision Your text
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===Lunar Laser Communication Demonstration===

===Lunar Laser Communication Demonstration===

{{main|Lunar Laser Communication Demonstration}}

{{main|Lunar Laser Communication Demonstration}}

[[File:LADEE's LLCD optical module rendering.jpg|thumb|[[Assembly modelling|CAD assembly]] depiction of the optical module of the LLCD]]

[[File:LADEE's LLCD optical module rendering.jpg|thumb|Depiction of the optical module of the LLCD]]

LADEE's ''Lunar Laser Communication Demonstration'' (LLCD) [[pulsed laser]] system conducted a successful test on October 18, 2013, transmitting data between the spacecraft and its ground station on Earth at a distance of {{convert|239000|mi|km|order=flip}}. This test set a [[downlink]] record of 622 [[megabit]]s per second (Mbps) from spacecraft to ground, and an "error-free data upload rate of 20 Mbps" from ground station to spacecraft.<ref name="parabolic 20131022" /> Tests were carried out over a 30-day test period.<ref>{{cite news |url=http://www.redorbit.com/news/space/1113034994/lunar-laser-communication-demonstration-reveals-bright-future-for-space-communication-122413/ |title=Lunar Laser Communication Demonstration Reveals Bright Future For Space Communication |work=NASA |publisher=Red Orbit |date=December 24, 2013 |access-date=October 12, 2014}}</ref>

LADEE's ''Lunar Laser Communication Demonstration'' (LLCD) [[pulsed laser]] system conducted a successful test on October 18, 2013, transmitting data between the spacecraft and its ground station on Earth at a distance of {{convert|239000|mi|km|order=flip}}. This test set a [[downlink]] record of 622 [[megabit]]s per second (Mbps) from spacecraft to ground, and an "error-free data upload rate of 20 Mbps" from ground station to spacecraft.<ref name="parabolic 20131022" /> Tests were carried out over a 30-day test period.<ref>{{cite news |url=http://www.redorbit.com/news/space/1113034994/lunar-laser-communication-demonstration-reveals-bright-future-for-space-communication-122413/ |title=Lunar Laser Communication Demonstration Reveals Bright Future For Space Communication |work=NASA |publisher=Red Orbit |date=December 24, 2013 |access-date=October 12, 2014}}</ref>



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* The Neutral Mass Spectrometer (NMS) team has been searching the data for exhaust gas species such as water, carbon monoxide and carbon dioxide (CO and CO<sub>2</sub>) as well as nitrogen (N<sub>2</sub>).<ref name="results Jan 2014" />

* The Neutral Mass Spectrometer (NMS) team has been searching the data for exhaust gas species such as water, carbon monoxide and carbon dioxide (CO and CO<sub>2</sub>) as well as nitrogen (N<sub>2</sub>).<ref name="results Jan 2014" />

* The Ultraviolet and Visible light Spectrometer (UVS) carried out a series of before/after observations looking for effects of both the landing and meteor showers. Analysis revealed an increase in sodium in the exosphere in connection with the Geminid meteor shower, as well as evidence of increased light scattering due to dust. The UVS also monitored emission lines of atomic oxygen, and saw emissions that may have indicated the presence of both iron (Fe) and titanium ([[Titanium|Ti]]), which were expected but they had never before been observed.<ref name="results Jan 2014" />

* The Ultraviolet and Visible light Spectrometer (UVS) carried out a series of before/after observations looking for effects of both the landing and meteor showers. Analysis revealed an increase in sodium in the exosphere in connection with the Geminid meteor shower, as well as evidence of increased light scattering due to dust. The UVS also monitored emission lines of atomic oxygen, and saw emissions that may have indicated the presence of both iron (Fe) and titanium ([[Titanium|Ti]]), which were expected but they had never before been observed.<ref name="results Jan 2014" />

*[[Helium-4|<sup>4</sup>He]], <sup>20</sup>[[Isotopes of neon|Ne]], and [[Isotopes of argon|<sup>40</sup>Ar]] gases were determined to be the most abundant species in the lunar exosphere.<ref name="update">{{Cite web |url=http://www.nasa.gov/ames/ladee/ladee-project-scientist-update-december-2014 |title=LADEE Project Scientist Update: December 2014 |publisher=NASA |first=Rick |last=Elphic |date=December 16, 2014 |access-date=July 26, 2015}}</ref><ref name="Texas 2014">{{cite conference |url=http://www.hou.usra.edu/meetings/lpsc2014/pdf/2677.pdf |title=The Lunar Atmosphere and Dust Environment Explorer (LADEE): Initial Science Results |conference=45th Lunar and Planetary Science Conference. The Woodlands, Texas. March 17–21, 2014. |publisher=Lunar and Planetary Institute |first1=R. C. |last1=Elphic |first2=B. |last2=Hine |first3=G. T. |last3=Delory |first4=J. S. |last4=Salute |first5=S. |last5=Noble |first6=A. |last6=Colaprete |first7=M. |last7=Horanyi |first8=P. |last8=Mahaffy |author9=LADEE Science Team |display-authors=5 |date=2014}}</ref> The helium and neon were found to be supplied by the [[solar wind]].<ref name="update"/>

*[[Helium]], [[argon]] and [[neon]] gases were determined to be the most abundant species in the lunar exosphere.<ref name="update">{{Cite web |url=http://www.nasa.gov/ames/ladee/ladee-project-scientist-update-december-2014 |title=LADEE Project Scientist Update: December 2014 |publisher=NASA |first=Rick |last=Elphic |date=December 16, 2014 |access-date=July 26, 2015}}</ref><ref name="Texas 2014">{{cite conference |url=http://www.hou.usra.edu/meetings/lpsc2014/pdf/2677.pdf |title=The Lunar Atmosphere and Dust Environment Explorer (LADEE): Initial Science Results |conference=45th Lunar and Planetary Science Conference. The Woodlands, Texas. March 17–21, 2014. |publisher=Lunar and Planetary Institute |first1=R. C. |last1=Elphic |first2=B. |last2=Hine |first3=G. T. |last3=Delory |first4=J. S. |last4=Salute |first5=S. |last5=Noble |first6=A. |last6=Colaprete |first7=M. |last7=Horanyi |first8=P. |last8=Mahaffy |author9=LADEE Science Team |display-authors=5 |date=2014}}</ref> The helium and neon were found to be supplied by the [[solar wind]].<ref name="update"/>

* On August 17, 2015, based on studies with the LADEE spacecraft, NASA scientists reported the detection of [[neon]] in the [[exosphere]] of the Moon.<ref name="NASA-20150817">{{cite web |last=Steigerwald |first=William |title=NASA's LADEE Spacecraft Finds Neon in Lunar Atmosphere |url=http://www.nasa.gov/content/goddard/ladee-lunar-neon |date=August 17, 2015 |work=[[NASA]] |access-date=August 18, 2015}}</ref>

* On August 17, 2015, based on studies with the LADEE spacecraft, NASA scientists reported the detection of [[neon]] in the [[exosphere]] of the Moon.<ref name="NASA-20150817">{{cite web |last=Steigerwald |first=William |title=NASA's LADEE Spacecraft Finds Neon in Lunar Atmosphere |url=http://www.nasa.gov/content/goddard/ladee-lunar-neon |date=August 17, 2015 |work=[[NASA]] |access-date=August 18, 2015}}</ref>



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