Zobrazeno 1 - 10
of 31
pro vyhledávání: '"Wolters, Stephen D"'
Autor:
Morlok, Andreas, Schiller, Benjamin, Weber, Iris, Daswani, Mohit Melwani, Stojic, Aleksandra N., Reitze, Maximilian P., Gramse, Tim, Wolters, Stephen D., Hiesinger, Harald, Grady, Monica M., Helbert, Jörn
Publikováno v:
In Planetary and Space Science 15 November 2020 193
Autor:
Wolters, Stephen D., Weissman, Paul R., Christou, Apostolis, Duddy, Samuel R., Lowry, Stephen C.
Infrared spectroscopy between 0.8 and 2.5 microns has been obtained for both components of three unbound asteroid pairs, using the NASA-IRTF with the SpeX instrument. Pair primary (2110) Moore-Sitterly is classified as an S-type following the Bus-DeM
Externí odkaz:
http://arxiv.org/abs/1401.5963
Autor:
Wolters, Stephen D., Hagene, Jon K., Sund, Arnt T., Bohman, Axel, Guthery, William, Sund, Bjornar T., Hagermann, Axel, Tomkinson, Tim, Romstedt, Jens, Morgan, Geraint H., Grady, Monica M.
We have designed and built a compact breadboard prototype instrument called WatSen: a combined ATR mid-IR spectrometer, fixed-focus microscope, and humidity sensor. The instrument package is enclosed in a rugged cylindrical casing only 26mm in diamet
Externí odkaz:
http://arxiv.org/abs/1303.3020
Autor:
Wolters, Stephen D., Rozitis, Ben, Duddy, Samuel R., Lowry, Stephen C., Green, Simon F., Snodgrass, Colin, Hainaut, Olivier R., Weissman, Paul
Asteroid (175706) 1996 FG3 is a binary asteroid and the baseline target for the proposed MarcoPolo-R sample-return mission. We present thermal IR photometry obtained with the ESO VLT+VISIR together with optical photometry obtained with the ESO NTT+EF
Externí odkaz:
http://arxiv.org/abs/1108.1831
A concept for an Impact Mitigation Preparation Mission, called Don Quijote, is to send two spacecraft to a Near-Earth Asteroid (NEA): an Orbiter and an Impactor. The Impactor collides with the asteroid while the Orbiter measures the resulting change
Externí odkaz:
http://arxiv.org/abs/1107.4229
Autor:
Wolters, Stephen D., Green, Simon F.
Publikováno v:
Mon.Not.Roy.Astron.Soc.400:204-218,2009
The Near-Earth Asteroid Thermal Model (NEATM, Harris, 1998) has proven to be a reliable simple thermal model for radiometric diameter determination. However NEATM assumes zero thermal emission on the night side of an asteroid. We investigate how this
Externí odkaz:
http://arxiv.org/abs/0905.1601
Autor:
Ball, Andrew J., Ulamec, Stephan, Dachwald, Bernd, Price, Michael E., Nadalini, Riccardo, Luethi, Benjamin, Wolters, Stephen D., Sheridan, Simon, Green, Simon F., Zarnecki, John C., D’Arrigo, Paolo, Seiferlin, Karsten, Kargl, Günter, Goerke, Nils
Publikováno v:
In Advances in Space Research 2009 43(2):317-324
Autor:
Morlok, A., Schiller, Benjamin, Weber, I., Melwani-Daswani, M, Stojic, A., Reitze, Maximilian P., Gramse, Tim, Wolters, Stephen D., Bauch, K.E., Hiesinger, Harald, Grady, Monica, Helbert, Jörn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1640::80c23250b66dfe343f013a56c1997da8
https://elib.dlr.de/138769/
https://elib.dlr.de/138769/
Autor:
Wolters, Stephen D
Increased physical characterisation of Near-Earth Asteroids (NEAs) is important for understanding their origin and evolution, the links between meteorites and their parent bodies, and for assessing the impact hazard. NEAs are also representative of s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c11fc46f498ee8a06347fbfd4494c019