LCROSS Mission Impact Observation
10.09.2009
The impact of the LCROSS payload into
the Lunar crater Cabeus was observed from the Via Capote Observatory.
Local conditions were generally good with high humidity and calm winds.
Seeing conditions were “good” to “very good”.
|
Temperature |
54F |
|
Wind |
Calm |
|
Humidity |
95% |
|
Barometric Pressure |
30.07 and
falling |
|
Conditions / Observations |
Heavy dewing
conditions, transparency deteriorated during observing run
|
The
observations were made through a Meade 14” SCT featuring an f/10 focal
ratio. The telescope mount is an LX200 tracking in “Lunar” mode. Focus
was maintained using an Optec temperature compensated focusing system. A
computerized focus run was preformed approximately 8 hours prior to
predicted impact using a background star.
Image data was collected using a Santa
Barbara Instruments ST-402 camera, cooled to -5 C. The image data was
collected “un-binned”. This configuration yielded an image scale of
approximately .5 arc seconds per pixel and a total field of view of
approximately 7 X 4 arc minutes. To accommodate the very bright
background of the lunar disk, three filters (blue, green, and yellow) were
stacked and inserted into the optical path of the camera so as to prevent
saturation. The camera was set to acquire data continuously with .1
second integration periods. All images were dark frame corrected. No
flat field frame corrections were required or applied. No other signal
processing was applied.
The observatory clock was synchronized
to NIST approximately 8 hours prior to predicted impact. Data was acquired
from 13 seconds prior to predicted impact until 739 seconds after impact.
652 individual images were acquired during the period spanning the
predicted impact.
There was no obvious indication of
impact from the data collected. Frame to frame variation induced by
seeing and variable transparency conditions produced some notable
candidates for suspected impact but closer examination of the data
discounted the possibility of these being anything other then artifacts of
the variable conditions. Attached are a few sample images, post and pre
impact with the target area highlighted in the first image.
Image Time 6 seconds before predicted
impact

Image Time 633 seconds after predicted
impact