Zobrazeno 1 - 4
of 4
pro vyhledávání: '"John R. Weirich"'
Autor:
Eric E. Palmer, John R. Weirich, Robert W. Gaskell, Diane Lambert, Tanner Campbell, Kris Drozd, Olivier S. Barnouin, Michael G. Daly, Kenneth Getzandanner, John N. Kidd Jr., Coralie D. Adam, Dante S. Lauretta
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 2, p 46 (2024)
Stereophotoclinometry (SPC) was the prime method of shape modeling for NASA’s OSIRIS-REx mission to asteroid Bennu. Here we describe the extensive testing conducted before launch to certify SPC as NASA Class B flight software, which not only valida
Externí odkaz:
https://doaj.org/article/23a4fb30c87d4d4b9be87816d4752944
Autor:
Eric E. Palmer, John R. Weirich, Robert W. Gaskell, Diane Lambert, Tanner Campbell, Kris Drozd, Olivier S. Barnouin, Michael G. Daly, Kenneth Getzandanner, John N. Kidd Jr., Coralie D. Adam, Dante S. Lauretta
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 2, p 47 (2024)
The OSIRIS-REx mission used stereophotoclinometry (SPC) to generate digital terrain models (DTMs) of its target asteroid, Bennu. Here we present a suite of preflight tests conducted to identify the observing geometry and number of images needed to cr
Externí odkaz:
https://doaj.org/article/9b554404ea8e4f26b3dcf1f623347be1
Autor:
John R. Weirich, Deborah L. Domingue, Frank C. Chuang, Amanda A. Sickafoose, Matthew D. Richardson, Eric E. Palmer, Robert W. Gaskell
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 11, p 212 (2023)
Lunar swirls have been traditionally considered to be unaffected by topographic changes. Yet, correlations between areas of high albedo and lower elevations are observed in regions of the Mare Ingenii swirl. Here, we apply similar techniques used at
Externí odkaz:
https://doaj.org/article/dbb2e9123f64435daaa4b7ac1a7ebd23
Autor:
Frank C. Chuang, Matthew D. Richardson, John R. Weirich, Amanda A. Sickafoose, Deborah L. Domingue
Publikováno v:
The Planetary Science Journal. 3:231
Lunar swirls are recognized as broad, bright albedo features in various regions of the Moon. These features are often separated by dark off-swirl lanes or terminate against the dark background, such as lunar maria. Prior mapping of swirls has been do