Your browser doesn't support javascript.
loading
Light curves and colours of the ejecta from Dimorphos after the DART impact.
Graykowski, Ariel; Lambert, Ryan A; Marchis, Franck; Cazeneuve, Dorian; Dalba, Paul A; Esposito, Thomas M; O'Conner Peluso, Daniel; Sgro, Lauren A; Blaclard, Guillaume; Borot, Antonin; Malvache, Arnaud; Marfisi, Laurent; Powell, Tyler M; Huet, Patrice; Limagne, Matthieu; Payet, Bruno; Clarke, Colin; Murabana, Susan; Owen, Daniel Chu; Wasilwa, Ronald; Fukui, Keiichi; Goto, Tateki; Guillet, Bruno; Huth, Patrick; Ishiyama, Satoshi; Kukita, Ryuichi; Mitchell, Mike; Primm, Michael; Randolph, Justus; Rivett, Darren A; Ryno, Matthew; Shimizu, Masao; Toullec, Jean-Pierre; Will, Stefan; Yue, Wai-Chun; Camilleri, Michael; Graykowski, Kathy; Janetzke, Ron; Janke, Des; Kardel, Scott; Loose, Margaret; Pickering, John W; Smith, Barton A; Transom, Ian M.
Afiliação
  • Graykowski A; SETI Institute, Carl Sagan Center, Mountain View, CA, USA. agraykowski@seti.org.
  • Lambert RA; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Marchis F; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Cazeneuve D; Unistellar, Marseille, France.
  • Dalba PA; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Esposito TM; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • O'Conner Peluso D; Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA, USA.
  • Sgro LA; Heising-Simons 51 Pegasi b Postdoctoral Fellow, New York City, NY, USA.
  • Blaclard G; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Borot A; Unistellar, Marseille, France.
  • Malvache A; Astronomy Department, University of California, Berkeley, CA, USA.
  • Marfisi L; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Powell TM; Centre for Astrophysics, University of Southern Queensland, Toowoomba, Queensland, Australia.
  • Huet P; SETI Institute, Carl Sagan Center, Mountain View, CA, USA.
  • Limagne M; Unistellar, Marseille, France.
  • Payet B; Unistellar, Marseille, France.
  • Clarke C; Unistellar, Marseille, France.
  • Murabana S; Unistellar, Marseille, France.
  • Owen DC; Unistellar, Marseille, France.
  • Wasilwa R; Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, CA, USA.
  • Fukui K; Unistellar Citizen Scientist, Le Tampon, France.
  • Goto T; Unistellar Citizen Scientist, Saint-Paul, Réunion.
  • Guillet B; Unistellar Citizen Scientist, La Rivière, Réunion.
  • Huth P; Armagh Observatory and Planetarium, College Hill, Armagh, UK.
  • Ishiyama S; The Travelling Telescope, Nairobi Planetarium, Nairobi, Kenya.
  • Kukita R; Unistellar Citizen Scientist, College Hill, UK.
  • Mitchell M; The Travelling Telescope, Nairobi Planetarium, Nairobi, Kenya.
  • Primm M; Unistellar Citizen Scientist, Nairobi, Kenya.
  • Randolph J; The Travelling Telescope, Nairobi Planetarium, Nairobi, Kenya.
  • Rivett DA; Unistellar Citizen Scientist, Nairobi, Kenya.
  • Ryno M; The Travelling Telescope, Nairobi Planetarium, Nairobi, Kenya.
  • Shimizu M; Unistellar Citizen Scientist, Nairobi, Kenya.
  • Toullec JP; Unistellar Citizen Scientist, Tsuchiura, Japan.
  • Will S; Unistellar Citizen Scientist, Osaka, Japan.
  • Yue WC; Unistellar Citizen Scientist, Caen, France.
  • Camilleri M; Community College of Allegheny County, Pittsburgh, PA, USA.
  • Graykowski K; Unistellar Citizen Scientist, Schenley, PA, USA.
  • Janetzke R; Unistellar Citizen Scientist, Chigasaki, Japan.
  • Janke D; Unistellar Citizen Scientist, Kajiki Aira, Japan.
  • Kardel S; Unistellar Citizen Scientist, Oklahoma City, OK, USA.
  • Loose M; Unistellar Citizen Scientist, Austin, TX, USA.
  • Pickering JW; Unistellar Citizen Scientist, Athens, GA, USA.
  • Smith BA; Unistellar Citizen Scientist, Lake Macquarie, New South Wales, Australia.
  • Transom IM; Unistellar Citizen Scientist, Milwaukee, WI, USA.
Nature ; 616(7957): 461-464, 2023 04.
Article em En | MEDLINE | ID: mdl-36858076
ABSTRACT
On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft struck Dimorphos, a satellite of the asteroid 65803 Didymos1. Because it is a binary system, it is possible to determine how much the orbit of the satellite changed, as part of a test of what is necessary to deflect an asteroid that might threaten Earth with an impact. In nominal cases, pre-impact predictions of the orbital period reduction ranged from roughly 8.8 to 17 min (refs. 2,3). Here we report optical observations of Dimorphos before, during and after the impact, from a network of citizen scientists' telescopes across the world. We find a maximum brightening of 2.29 ± 0.14 mag on impact. Didymos fades back to its pre-impact brightness over the course of 23.7 ± 0.7 days. We estimate lower limits on the mass contained in the ejecta, which was 0.3-0.5% Dimorphos's mass depending on the dust size. We also observe a reddening of the ejecta on impact.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nature Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nature Ano de publicação: 2023 Tipo de documento: Article País de afiliação: Estados Unidos