Of course everyone reading this knows about the #NASASocial event for the launch of the LADEE mission to Lunar orbit happening this week on Thursday (9/5) and Friday (9/6). Follow NASASocial/lists/ladee-launch-social plus @NASA_Wallops, @NASALADEE, @NASAAmes, @NASAGoddard, and also @LRO_NASA for updates.
A nice piece of Wallops history was raised by @TeresaR_WV: “Explorer 9 was the first spacecraft placed in orbit by an all-solid rocket and the first spacecraft successfully launched into orbit from Wallops Island.” (1961, NSSDC).
The LADEE social will be covering a huge range of subjects, including the following.
- LADEE Science
- Minotaur-V launch of LADEE
- Wallops Island Launch Pads and Range Control
- Very High Altitude Balloon fabrication and flying
- Sounding Rocket flying
- Global Hawks Airborne Science
The LADEE mission will be collecting data on the Lunar Exosphere, specifically tightening the boundaries on gas and dust types and quantities found at altitudes under 50 km so that future work can develop an understanding of the surface boundary exospheric processes that occur on inert rocky bodies like the Moon and Mercury. And the LADEE mission will be flight qualifying the LLCD free space optical communications link. Data collection in the Lunar Exosphere will employ three instruments.
The Neutral Mass Spectrometer (NMS) determines captured (Lunar Exosphere) gas particle types (element) using a kind of electromagnetic filter called an RF Quadrupole or Quadrupole mass analyzer, or Mass Spectrometer. Instruments very similar to this one have flown on many deep space missions including CASSINI. In determining gas types with fairly high frequency (many per second), gas quantity and distribution can be determined over time.
The Ultraviolet – Visible Spectrometer (UVS) will determine observed (Lunar Exosphere) gas types by the characteristic electromagnetic emission spectra of gas particles impacted by solar radiation. It is also capable of a few additional modes (that I haven’t groked yet) that provide information about gas and dust processes in the exosphere.
The Lunar Dust Experiment (LDEX) captures larger “dust” particles to determine composition and distribution over time, not entirely unlike the NMS. Also not entirely unlike the NMS, it employs an electromagnetic process to do so.
The NMS and LDEX are forward facing, while the UVS is rearward facing, in LADEE’s direction of flight. That is, LADEE flies sideways relative to its Lunar Capture rocket engine which it points out of the way otherwise.
The NASA TV broadcast schedule includes events on Thursday and Friday.
September 5, Thursday
10 -11:30 a.m. – NASA Social for LADEE Mission Live from the Wallops Flight Facility – HQ/WFF (Education Channel)
3 p.m. – LADEE Prelaunch Mission Briefing – HQ/WFF (All Channels)
4 p.m. – LADEE Mission Science and Technology Demonstration Briefing – HQ/WFF (All Channels)
September 6, Friday
6-10 a.m. –Live Interviews on the LADEE Mission – HQ/WFF (All Channels)
4-6 p.m. – Live Interviews on LADEE Mission – HQ/WFF (All Channels)
9:30 p.m. – Live Launch Coverage and Commentary on LADEE Mission – HQ/GSFC/WFF (Public and Media Channels)
9:30 p.m. – Simulcast of NASA EDGE Live Webcast of LADEE Mission and Launch – LARC/HQ/WFF (Education Channel)
September 7, Saturday
2 a.m. – LADEE Post Launch News Conference –HQ/WFF (All Channels)