Lcross_palomar < Palomar/PalmLGS

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---+++ Oct. 9, 2009 UT LCROSS Impact Imaging
---++++ Preliminary Results
Palomar AO image of Cabeus crater 10s after Centaur impact:
<a href="%ATTACHURLPATH%/Palomar_ao_bouchez_10s_after_impact.png"><img src="%ATTACHURLPATH%/Palomar_ao_bouchez_10s_after_impact.png" alt="Palomar_ao_bouchez_10s_after_impact.png" height='450'></a><br>
<a href="%ATTACHURLPATH%/Palomar_ao_bouchez_15s_after_impact.png">... and 15s after impact.</a>  No obvious detection of an impact ejecta plume.

[[%ATTACHURL%/lcross_palomar.mpg][ *Palomar AO movie of the LCROSS impact (19 Mb MPEG)* ]]

---++++ Contact Information
   * Palomar dataroom phone: 760-642-2105
   * !WebEx telecon starts at 18:30 10/8/09 PDT.
   * [[%ATTACHURL%/LCROSS_Observatory_Status_Sheet_6Oct.doc][Participating Observatories (.doc)]]

---++++ Schedule (Times UT, updated 10/6/09)
   * ~02:00 Spacecraft separation
   * 08:30 Acquire Cabeus crater; determine best feature to use for AO lock
   * 10:30 Acquire 1st set of sky background frames
   * 11:00 Begin impact imaging sequence
   * *11:31:19 Centaur impact*
   * 11:35:45 Shepherding spacecraft impact
   * 11:50 End impact imaging sequence, acquire 2nd set of sky background frames
   * 14:00 NASA ARC press conference (submit graphics by 12:30)

---++++ Observing Plan
Our goal is to image the evolution of the LCROSS debris plume at the highest possible spatial resolution.  We plan to use the Palomar Adaptive Optics system to lock on a bright lunar feature, probably a crater wall or mountain peak, near the predicted impact location.  Full AO correction should provide spatial resolution of ~0.1 arcseconds (180 meters at Cabeus crater) across the 40 arcsecond (71 km) field of view of the PHARO near-infrared camera.

The debris curtain is expected to expand at ~150 m/s, reaching maximum brightness after ~60s at a diameter of ~20 km.  We will acquire 1.4s integrations every 2.8s, thus providing a ~40 frame movie of the expanding debris plume during its highest density phase.  We will observe at K band (2.1 microns), to maximize AO correction and sensitivity to large particles.

We have allocated 2 hrs (8:30-10:30 UT) to locate Cabeus crater and test surrounding features for that providing the best AO correction.  We will then offset to blank sky to acquire bias/background frames, and begin our impact imaging sequence at 11:00 UT.  We intend to continue the image sequence through impact and for at least 15 minutes after Centaur impact.

---++++ Finder Charts
PHARO 40" field overlaid on  NASA GSFC visualization as seen from Palomar.
     <a href="%ATTACHURLPATH%/pharo_field.png"><img src="%ATTACHURLPATH%/pharo_field.png" alt="pharo_field.png" height='400' ></a><br>
<br>
Gemini finder chart
     <a href="%ATTACHURLPATH%/Gemini_finder_chart.png"><img src="%ATTACHURLPATH%/Gemini_finder_chart.png" alt="Gemini_finder_chart.png" height='400' ></a>

---++++ Ephemeris, Timelines, Etc.
   * Range to impact site is 3.66936 x 10^5 km.
   * [[%ATTACHURL%/cabeus_ephem.txt][cabeus_ephem.txt]]: Ephemeris for moon lat: 310.95, lon: -84.70, alt:0 km.

   * [[%ATTACHURL%/LCROSS_Observatory_Status_Sheet_6Oct.doc][NASA ARC ground-based coordination timeline (.xls)]]

---++++ Links
   * [[http://lcross.arc.nasa.gov/][NASA ARC LCROSS web pages]]

Attachments

Topic attachments
I	Attachment	History	Action	Size	Date	Who
png	Gemini_finder_chart.png	r2 r1	manage	1027.4 K	2009-10-08 - 22:01	UnknownUser
xls	LCROSS_Observation_Campaign_Timeline_6Oct.xls	r1	manage	20.5 K	2009-10-07 - 05:41	UnknownUser
doc	LCROSS_Observatory_Status_Sheet_6Oct.doc	r1	manage	43.5 K	2009-10-07 - 05:41	UnknownUser
png	Palomar_ao_bouchez_10s_after_impact.png	r1	manage	318.8 K	2009-10-09 - 14:52	UnknownUser
png	Palomar_ao_bouchez_15s_after_impact.png	r1	manage	318.2 K	2009-10-09 - 14:53	UnknownUser
txt	cabeus_ephem.txt	r1	manage	29.1 K	2009-10-07 - 00:00	UnknownUser
mpg	lcross_palomar.mpg	r1	manage	19207.9 K	2009-10-10 - 07:21	UnknownUser
png	pharo_field.png	r1	manage	786.5 K	2009-10-07 - 20:30	UnknownUser

Topic revision: r9 - 2009-10-10 - AntoninBouchez

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