(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model
A 167-parameter, 3-D shape model of Castalia, obtained from inversion of delay-Doppler images, constrained the object's subradar latitude on the date of the observations by defining an annular sky region that contains Castalia's pole. We have used the shape model and nominal Hapke paramete...
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ftnasajpl:oai:trs.jpl.nasa.gov:2014/34590 2023-05-15T18:22:27+02:00 (abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model Hudson, R.S. Ostro, S.J. Harris, A.W. 2004-10-06 80902 bytes application/pdf http://hdl.handle.net/2014/34590 en_US eng Washington, DC 94-0945 http://hdl.handle.net/2014/34590 asteroid Castalia shape radar 3-D model optical lightcurves 2004 ftnasajpl 2021-12-23T13:20:24Z A 167-parameter, 3-D shape model of Castalia, obtained from inversion of delay-Doppler images, constrained the object's subradar latitude on the date of the observations by defining an annular sky region that contains Castalia's pole. We have used the shape model and nominal Hapke parameters for S asteroids to model Castalia lightcurves obtained at Table Mountain Observatory on August 23-25, 1989, at solar phase angles ranging from 58° to 90°. This investigation defines the projected pole's azimuthal orientation around the radar line of sight and therefore yields a least-squares estimate of the orientation of Castalia's north or south pole; there is insufficient geometric leverage to distinguish the rotation sense or to estimate values of Hapke parameters. The model lightcurves match the TMO data surprisingly well, given the modest number of shape parameters in the model and the fact that part of the asteroid was not seen by the radar. Other/Unknown Material South pole JPL Technical Report Server South Pole Table Mountain ENVELOPE(69.031,69.031,-48.668,-48.668) |
institution |
Open Polar |
collection |
JPL Technical Report Server |
op_collection_id |
ftnasajpl |
language |
English |
topic |
asteroid Castalia shape radar 3-D model optical lightcurves |
spellingShingle |
asteroid Castalia shape radar 3-D model optical lightcurves Hudson, R.S. Ostro, S.J. Harris, A.W. (abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
topic_facet |
asteroid Castalia shape radar 3-D model optical lightcurves |
description |
A 167-parameter, 3-D shape model of Castalia, obtained from inversion of delay-Doppler images, constrained the object's subradar latitude on the date of the observations by defining an annular sky region that contains Castalia's pole. We have used the shape model and nominal Hapke parameters for S asteroids to model Castalia lightcurves obtained at Table Mountain Observatory on August 23-25, 1989, at solar phase angles ranging from 58° to 90°. This investigation defines the projected pole's azimuthal orientation around the radar line of sight and therefore yields a least-squares estimate of the orientation of Castalia's north or south pole; there is insufficient geometric leverage to distinguish the rotation sense or to estimate values of Hapke parameters. The model lightcurves match the TMO data surprisingly well, given the modest number of shape parameters in the model and the fact that part of the asteroid was not seen by the radar. |
author |
Hudson, R.S. Ostro, S.J. Harris, A.W. |
author_facet |
Hudson, R.S. Ostro, S.J. Harris, A.W. |
author_sort |
Hudson, R.S. |
title |
(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
title_short |
(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
title_full |
(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
title_fullStr |
(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
title_full_unstemmed |
(abstract) Asteroid 4769 Casalia: Intrepretation of Optical Lightcurves Using a Radar-Derived Shape Model |
title_sort |
(abstract) asteroid 4769 casalia: intrepretation of optical lightcurves using a radar-derived shape model |
publishDate |
2004 |
url |
http://hdl.handle.net/2014/34590 |
long_lat |
ENVELOPE(69.031,69.031,-48.668,-48.668) |
geographic |
South Pole Table Mountain |
geographic_facet |
South Pole Table Mountain |
genre |
South pole |
genre_facet |
South pole |
op_relation |
Washington, DC 94-0945 http://hdl.handle.net/2014/34590 |
_version_ |
1766201859553361920 |