Whipple (spacecraft) explained

Whipple was a proposed space observatory in the NASA Discovery Program.[1] The observatory would try to search for objects in the Kuiper belt and the theorized Oort cloud by conducting blind occultation observations.[2] Although the Oort cloud was hypothesized in the 1950s, it has not yet been directly observed.[2] The mission would attempt to detect Oort cloud objects by scanning for brief moments where the objects would block the light of background stars.[2]

In 2011, three finalists were selected for the 2016 Discovery Program, and Whipple was not among them, but it was awarded funding to continue its technological development efforts.[3]

Description

Whipple would orbit in a halo orbit around the Earth–Sun and have a photometer that would try to detect Oort cloud and Kuiper belt objects (KBOs) by recording their transits of distant stars.[1] It would be designed to detect objects out to . Some of the mission goals included directly detecting the Oort cloud for the first time and determining the outer limit of the Kuiper belt. Whipple would be designed to detect objects as small as a kilometer (half a mile) across at a distance of 2order=flipNaNorder=flip. Its telescope would need a relatively wide field of view and fast recording cadence to capture transits that may last only seconds.[4]

In 2011, Whipple was one of three proposals to win a technology development award in a Discovery Program selection.[5] The design proposed was a catadioptric Cassegrain telescope with a 77-centimeter aperture (30.3 inches).[6] It would have a wide field of view with a fast read-out CMOS detector to achieve the desired time and photometric sensitivity.[7]

The smallest KBO yet detected was discovered in 2009 by poring over data from the Hubble Space Telescope's fine guidance sensors.[8] Astronomers detected a transit of an object against a distant star, which, based on the duration and amount of dimming, was calculated to be a KBO about 3200feet in diameter. It has been suggested that the Kepler observatory may be able to detect objects in the Oort cloud by their occultation of background stars.[9]

See also

External links

Notes and References

  1. Web site: Alcock . Charles . Brown . Michael . Tom . Gauron . Cate . Heneghan . The Whipple Mission Exploring the Oort cloud and the Kuiper Belt . https://web.archive.org/web/20151117031224/http://whipple.cfa.harvard.edu/inc/documents/Alcock_AGUPoster_2014dec.pdf . November 17, 2015.
  2. Alcock. C.. Brown. M. E.. Gauron. T.. Heneghan. C.. Holman. M. J.. Kenter. A.. Kraft. R.. Lee. R.. Livingston. J.. 2014-12-01. The Whipple Mission: Exploring the Kuiper Belt and the Oort Cloud. 2014AGUFM.P51D3977A. AGU Fall Meeting Abstracts. 51. P51D–3977.
  3. Web site: NASA Selects 3 Finalists for 2016 Discovery Mission . SpaceNews.com . 27 December 2018 . 6 May 2011.
  4. https://www.osapublishing.org/abstract.cfm?uri=IODC-2014-IM3A.3 A Fast, Wide Field of View, Catadioptric Telescope for Whipple
  5. Web site: NASA Selects 'Whipple' Mission for Technology Development . www.space-travel.com . 27 December 2018 . May 10, 2011.
  6. Web site: High Energy Astrophysics. Group. CfA Web Services. whipple.cfa.harvard.edu. 2018-01-27.
  7. Web site: Alcock . Charles . Whipple: Exploring the Solar System beyond Neptune Using a Survey for Occultations of Bright Stars . Solar System Exploration: NASA Science . 27 December 2018.
  8. Web site: HubbleSite: News - Hubble Finds Smallest Kuiper Belt Object Ever Seen. hubblesite.org. 2018-01-27.
  9. 0912.0948. 2010ApJ...711L...7O. Detectability of Oort Cloud Objects Using Kepler. The Astrophysical Journal. 711. 1. L7. Ofek. Eran O. Nakar. Ehud. 2010. 10.1088/2041-8205/711/1/L7. 119240916.