O
Olivier S. Barnouin
Researcher at Johns Hopkins University Applied Physics Laboratory
Publications - 230
Citations - 7895
Olivier S. Barnouin is an academic researcher from Johns Hopkins University Applied Physics Laboratory. The author has contributed to research in topics: Asteroid & Impact crater. The author has an hindex of 40, co-authored 211 publications receiving 5364 citations. Previous affiliations of Olivier S. Barnouin include Johns Hopkins University.
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Journal ArticleDOI
OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
Dante S. Lauretta,S. S. Balram-Knutson,E. C. Beshore,William V. Boynton,C. Drouet d'Aubigny,Daniella DellaGiustina,H. L. Enos,Dathon Golish,Carl Hergenrother,Ellen S. Howell,Carina Bennett,E. T. Morton,Michael C. Nolan,Bashar Rizk,H. L. Roper,Arlin E. Bartels,Brent J. Bos,Jason P. Dworkin,D. E. Highsmith,D. A. Lorenz,Lucy F. Lim,Ronald G. Mink,Michael C. Moreau,Joseph A. Nuth,D. C. Reuter,Amy Simon,Edward B. Bierhaus,B. H. Bryan,Ronald-Louis Ballouz,Olivier S. Barnouin,Richard P. Binzel,William F. Bottke,Victoria E. Hamilton,Kevin J. Walsh,S. R. Chesley,Philip R. Christensen,Beth E. Clark,Harold C. Connolly,M. K. Crombie,Michael Daly,Josh Emery,Timothy J. McCoy,Jay W. McMahon,Daniel J. Scheeres,Scott Messenger,Keiko Nakamura-Messenger,Kevin Righter,Scott A. Sandford +47 more
TL;DR: The OSIRIS-REx spacecraft departed for near-Earth asteroid (101955) Bennu via an United Launch Alliance Atlas V 411 evolved expendable launch vehicle at 7:05 p.m. EDT on September 8, 2016, on a seven-year journey to return samples from Bennu as discussed by the authors.
Journal ArticleDOI
The Pluto system: Initial results from its exploration by New Horizons.
S. A. Stern,Fran Bagenal,Kimberly Ennico,G. R. Gladstone,William M. Grundy,William B. McKinnon,J. M. Moore,Catherine B. Olkin,John R. Spencer,Harold A. Weaver,Leslie A. Young,Tom Andert,Jane M. Andrews,M. E. Banks,B. Bauer,Jeremy Bauman,Olivier S. Barnouin,Peter D. Bedini,K. B. Beisser,Ross A. Beyer,S. Bhaskaran,Richard P. Binzel,Emma Birath,Mike Bird,D. J. Bogan,Alice Bowman,Veronica J. Bray,M. Brozovic,C. Bryan,Matthew R. Buckley,Marc W. Buie,Bonnie J. Buratti,Stewart Bushman,Andrew B. Calloway,Brian Carcich,Andrew F. Cheng,Steven J. Conard,C. A. Conrad,Jason C. Cook,Dale P. Cruikshank,O. S. Custodio,C. M. Dalle Ore,C. C. Deboy,Zach Dischner,Philip J. Dumont,Alissa M. Earle,H. A. Elliott,J. Ercol,Carolyn M. Ernst,Tiffany J. Finley,Sarah H. Flanigan,Glen H. Fountain,M. J. Freeze,Thomas K. Greathouse,James L. Green,Yanping Guo,Matthias Hahn,Douglas P. Hamilton,Sarah A. Hamilton,Jennifer Hanley,A. Harch,H. M. Hart,Chris B. Hersman,A. Hill,Matthew E. Hill,David P. Hinson,Mark E. Holdridge,Mihaly Horanyi,Alan D. Howard,Carly Howett,Coralie D. Jackman,Robert A. Jacobson,D. E. Jennings,Joshua A. Kammer,H. K. Kang,David E. Kaufmann,Peter Kollmann,Stamatios M. Krimigis,David Y. Kusnierkiewicz,Tod R. Lauer,J. E. Lee,K. L. Lindstrom,Ivan Linscott,Carey M. Lisse,Allen W. Lunsford,V. A. Mallder,Nicole Martin,David J. McComas,Ralph L. McNutt,Douglas S. Mehoke,Thomas Mehoke,E. D. Melin,Max Mutchler,Derek S. Nelson,Francis Nimmo,Jorge I. Nunez,A. C. Ocampo,William M. Owen,Martin Paetzold,B. Page,Alex Parker,Joel Wm. Parker,Frederic Pelletier,J. Peterson,Nickalaus Pinkine,M. Piquette,Simon B. Porter,Silvia Protopapa,Jillian Redfern,Harold J. Reitsema,D. C. Reuter,James H. Roberts,Stuart J. Robbins,Gabe Rogers,Debi Rose,Kirby Runyon,Kurt D. Retherford,M. G. Ryschkewitsch,Paul M. Schenk,Eric Schindhelm,B. Sepan,Mark R. Showalter,Kelsi N. Singer,M. Soluri,Dale Stanbridge,Andrew J. Steffl,Darrell F. Strobel,T. Stryk,Michael E. Summers,Jamey Szalay,M. B. Tapley,A. Taylor,H. W. Taylor,Henry B. Throop,Constantine Tsang,G. L. Tyler,Orkan M. Umurhan,A. J. Verbiscer,M. H. Versteeg,Michael Vincent,R. W. Webbert,S. Weidner,G. Weigle,Oliver L. White,Karl Whittenburg,B. G. Williams,Kaj E. Williams,S. P. Williams,W. W. Woods,Amanda M. Zangari,Eric J. Zirnstein +150 more
TL;DR: The New Horizons encounter revealed that Pluto displays a surprisingly wide variety of geological landforms, including those resulting from glaciological and surface-atmosphere interactions as well as impact, tectonic, possible cryovolcanic, and mass-wasting processes.
Journal ArticleDOI
Hayabusa2 arrives at the carbonaceous asteroid 162173 Ryugu—A spinning top–shaped rubble pile
Sei-ichiro Watanabe,Sei-ichiro Watanabe,Masatoshi Hirabayashi,Naru Hirata,Na. Hirata,Rina Noguchi,Yuri Shimaki,H. Ikeda,Eri Tatsumi,Makoto Yoshikawa,Makoto Yoshikawa,Shota Kikuchi,Hikaru Yabuta,Tomoki Nakamura,Shogo Tachibana,Shogo Tachibana,Yoshiaki Ishihara,Tomokatsu Morota,Kohei Kitazato,Naoya Sakatani,Koji Matsumoto,Koji Wada,Hiroki Senshu,C. Honda,Tatsuhiro Michikami,Hiroshi Takeuchi,Hiroshi Takeuchi,Toru Kouyama,R. Honda,Shingo Kameda,Tetsuharu Fuse,Hideaki Miyamoto,Goro Komatsu,S. Sugita,Tatsuaki Okada,Tatsuaki Okada,Noriyuki Namiki,Masahiko Arakawa,Masateru Ishiguro,Masanao Abe,Masanao Abe,Robert Gaskell,Eric Palmer,Olivier S. Barnouin,Patrick Michel,A. S. French,Jay W. McMahon,Daniel J. Scheeres,Paul A. Abell,Yukio Yamamoto,Yukio Yamamoto,Satoshi Tanaka,Satoshi Tanaka,Kei Shirai,Moe Matsuoka,Manabu Yamada,Y. Yokota,Y. Yokota,H. Suzuki,Kosuke Yoshioka,Yuichiro Cho,Naoki Nishikawa,T. Sugiyama,Hideaki Kikuchi,Ryodo Hemmi,Tomohiro Yamaguchi,Naoko Ogawa,Go Ono,Yuya Mimasu,Kent Yoshikawa,T. Takahashi,Yuto Takei,Atsushi Fujii,Chikako Hirose,Takahiro Iwata,Takahiro Iwata,Masahiro Hayakawa,Satoshi Hosoda,Osamu Mori,Hirotaka Sawada,Takanobu Shimada,Stefania Soldini,Hajime Yano,Hajime Yano,Ryudo Tsukizaki,M. Ozaki,M. Ozaki,Yuichi Iijima,K. Ogawa,Masaki Fujimoto,T. M. Ho,Aurelie Moussi,Ralf Jaumann,J. P. Bibring,Christian Krause,Fuyuto Terui,Takanao Saiki,Satoru Nakazawa,Yoshiyuki Tsuda,Yoshiyuki Tsuda +99 more
TL;DR: The Hayabusa2 spacecraft measured the mass, size, shape, density, and spin rate of asteroid Ryugu, showing that it is a porous rubble pile, and observations of Ryugu's shape, mass, and geomorphology suggest that Ryugu was reshaped by centrifugally induced deformation during a period of rapid rotation.
Journal ArticleDOI
Initial observations from the Lunar Orbiter Laser Altimeter (LOLA)
David E. Smith,David E. Smith,Maria T. Zuber,Gregory A. Neumann,Frank G. Lemoine,Erwan Mazarico,Mark H. Torrence,Jan F. McGarry,David D. Rowlands,James W. Head,Thomas H. Duxbury,Oded Aharonson,Paul G. Lucey,Mark S. Robinson,Olivier S. Barnouin,John F. Cavanaugh,Xiaoli Sun,Peter Liiva,D. Mao,James C. Smith,Arlin E. Bartels +20 more
TL;DR: LOLA's initial global data sets as well as the first high-resolution digital elevation models (DEMs) of polar topography are described in this article, where LOLA has also provided the highest resolution global maps yet produced of slopes, roughness and the 1064-nm reflectance of the lunar surface.
Journal ArticleDOI
The geomorphology, color, and thermal properties of Ryugu: Implications for parent-body processes
Seiji Sugita,Seiji Sugita,Rie Honda,Tomokatsu Morota,Shingo Kameda,Hirotaka Sawada,Eri Tatsumi,Manabu Yamada,C. Honda,Yasuhiro Yokota,Yasuhiro Yokota,Toru Kouyama,Naoya Sakatani,K. Ogawa,H. Suzuki,Tatsuaki Okada,Tatsuaki Okada,Noriyuki Namiki,Satoshi Tanaka,Satoshi Tanaka,Yuichi Iijima,Kosuke Yoshioka,Masahiro Hayakawa,Yuichiro Cho,Moe Matsuoka,Naru Hirata,Hideaki Miyamoto,Deborah L. Domingue,Masatoshi Hirabayashi,Tomoki Nakamura,Takahiro Hiroi,Tatsuhiro Michikami,Patrick Michel,Ronald-Louis Ballouz,Ronald-Louis Ballouz,Olivier S. Barnouin,Carolyn M. Ernst,Stefan Schröder,Hideaki Kikuchi,Ryodo Hemmi,Goro Komatsu,Goro Komatsu,T. Fukuhara,Makoto Taguchi,Takehiko Arai,Hiroki Senshu,Hirohide Demura,Yoshiko Ogawa,Yuri Shimaki,Tomohiko Sekiguchi,T. G. Müller,Axel Hagermann,Takahide Mizuno,Hirotomo Noda,Koji Matsumoto,R. Yamada,Yoshiaki Ishihara,H. Ikeda,Hiroshi Araki,K. Yamamoto,Shinsuke Abe,Fumi Yoshida,A. Higuchi,Sho Sasaki,S. Oshigami,Seiitsu Tsuruta,Kazuyoshi Asari,Seiichi Tazawa,M. Shizugami,J. Kimura,Toshimichi Otsubo,Hikaru Yabuta,Sunao Hasegawa,Masateru Ishiguro,Shogo Tachibana,Eric Palmer,Robert Gaskell,L. Le Corre,Ralf Jaumann,Katharina A. Otto,Nicole Schmitz,Paul A. Abell,M. A. Barucci,Michael E. Zolensky,Faith Vilas,Florian Thuillet,C. Sugimoto,N. Takaki,Yutaka Suzuki,Hiroaki Kamiyoshihara,Masato Okada,Kenji Nagata,Masaki Fujimoto,Makoto Yoshikawa,Makoto Yoshikawa,Yukio Yamamoto,Yukio Yamamoto,Kei Shirai,Rina Noguchi,Naoko Ogawa,Fuyuto Terui,Shota Kikuchi,Tomohiro Yamaguchi,Yusuke Oki,Yuki Takao,Hiroshi Takeuchi,Go Ono,Yuya Mimasu,Kent Yoshikawa,T. Takahashi,Yuto Takei,Atsushi Fujii,Chikako Hirose,Satoru Nakazawa,Satoshi Hosoda,Osamu Mori,Takanobu Shimada,Stefania Soldini,Takahiro Iwata,Takahiro Iwata,Masanao Abe,Masanao Abe,Hajime Yano,Hajime Yano,Ryudo Tsukizaki,M. Ozaki,M. Ozaki,Kazutaka Nishiyama,Takanao Saiki,Sei-ichiro Watanabe,Sei-ichiro Watanabe,Yoshiyuki Tsuda,Yoshiyuki Tsuda +132 more
TL;DR: Spectral observations and a principal components analysis suggest that Ryugu originates from the Eulalia or Polana asteroid family in the inner main belt, possibly via more than one generation of parent bodies.