Article (Scientific journals)
Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches
Mennesson, Bertrand; Kennedy, G.; Ertel, S. et al.
2019In Bulletin of the American Astronomical Society, 51 (3), p. 324
 

Files


Full Text
324_mennesson.pdf
Author preprint (398.43 kB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Keywords :
Exoplanet; Exozodiacal dust
Abstract :
[en] The brightness and spatial distribution of warm ( 200K) dust structures located within a few AU We motivate and identify here the main instrumental / observational advances required to gain further insights into the origins of exozodiacal dust clouds and better understand their impact on planetary habitability and habitability searches.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Mennesson, Bertrand;  California Institute of Technology > Jet Propulsion Laboratory
Kennedy, G.
Ertel, S.
Wyatt, M.
Defrere, Denis ;  Université de Liège - ULiège > CSL (Centre Spatial de Liège)
Debes, J.
Stark, C.
Kasdin, J.
Macintosh, B.
Hinz, P.
Bailey, V.
Stapelfeldt, K.
Mawet, D.
Scott, N.
Roberge, A.
Lisse, C.
Lyra, W.
Hasegawa, Y.
Gaspar, A.
Danchi, W.
Millan-Gabet, R.
Haniff, C.
Skemer, A.
Serabyn, E.
Stone, J.
Bryden, G.
More authors (16 more) Less
Language :
English
Title :
Interplanetary dust around main sequence stars: origin, magnitude, and implications for exoplanet habitability searches
Publication date :
01 May 2019
Journal title :
Bulletin of the American Astronomical Society
ISSN :
0002-7537
eISSN :
2330-9458
Publisher :
American Astronomical Society, New York, United States - New York
Special issue title :
Astro2020: Decadal Survey on Astronomy and Astrophysics, science white papers, no. 324
Volume :
51
Issue :
3
Pages :
324
Available on ORBi :
since 13 August 2019

Statistics


Number of views
98 (3 by ULiège)
Number of downloads
53 (1 by ULiège)

Bibliography


Similar publications



Contact ORBi