OCA–DLR Asteroid Survey: Difference between revisions

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The '''OCA-DLR Asteroid Survey''' ('''ODAS''') was a European scientific project to search for [[asteroid]]s and [[comet]]s.<ref name="ODAS">{{cite web | last = Hahn | first = Gerhard | date = 2006-07-17 | url = http://earn.dlr.de/odas/ | title = O.D.A.S. Home Page | publisher = European Asteroid Research Node | accessdate = 2006-08-13 }}</ref> This project was the joint work of the [[Observatoire de la Côte d'Azur]] (OCA) in France and the [[Deutschen Zentrum für Luft- und Raumfahrt]] (DLR) in [[Germany]]. They operated in cooperation with a global effort regarding [[Near-Earth object]]s that was begun by the Working Group on Near-Earth Objects, a component of the [[International Astronomical Union]].<ref name="ODAS" />

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The '''OCA-DLR Asteroid Survey''' ('''ODAS''') was an [[astronomical survey]] to search for [[small Solar System bodies]] focusing on [[near-Earth object]]s in the late 1990s. This European scientific project – a collaboration between the French [[Observatoire de la Côte d'Azur]] (OCA) and the [[German Aerospace Center]] (DLR) – discovered a total of 956 [[asteroids]] and 1 [[comet]] during its course.<ref name="ODAS" />
This project began October 1996 and ceased observations in April 1999 for a refurbishing. However the telescope has not been reopened since that time.<ref>{{cite web | last = Paine | first = Michael | date = 2000-04-26 | url = http://www.space.com/news/japan_spacewatch_000426.html | title = Bigger Telescopes Seek Killer Asteroids | publisher = space.com | accessdate = 2006-08-13 }}</ref>


ODAS operated in cooperation with a global effort regarding [[Near-Earth object]]s that was begun by the Working Group on Near-Earth Objects, a component of the [[International Astronomical Union]].<ref name="ODAS" /> The project began October 1996 and ceased observations in April 1999 for a refurbishing. However the telescope has not been reopened since that time.<ref name="Space.com" /> Survey observations were made during the 15 days each month when moon light was at a minimum, during the first and last quarters of the lunar month.<ref name="ODAS" /> The operation used a 90&nbsp;cm [[Schmidt telescope]] of the OCA at Calern, near the city of [[Nice, France|Nice]] in southeastern France. A combination of a [[charge-coupled device|CCD]] camera<ref name="Maury-1998" /> and a software package<ref name="Hahn-1998" /> were used for automated detection of moving objects.
Survey observations were made during the 15 days each month when moon light was at a minimum, during the first and last quarters of the lunar month.<ref name="ODAS" /> The operation used a 90&nbsp;cm [[Schmidt telescope]] located near [[Nice, France]]. A combination of a [[charge-coupled device|CCD]] camera<ref>{{cite conference | author=A. Maury | author2=J.P. Ragey | author3=H. Viot| author4=M. Harald | author5=T. Behnke | date = 1998 | title =Converting a Schmidt Telescope to CCDs: the OCA/DLR Asteroid Survey | booktitle =Optical Detectors for Astronomy : Proceedings of an ESO CCD workshop held in Garching, Germany, October 8–10, 1996 | editor = James W. Beletic |editor2=Paola Amico | publisher = Kluwer Academic Publishers | location = Boston, Mass. | pages = 239 | url =http://adsabs.harvard.edu/abs/1998oda..conf..239M | accessdate =2006-08-13 }}</ref> and a software package<ref>{{cite journal | last = Hahn | first = Gerhard | title=Image processing and astrometric reduction routines of the OCA-DLR Asteroid Survey (O.D.A.S.) | journal=Acta Historica Astronomiae | date=1999 | volume=6 | pages=174 | bibcode=1999AcHA....6..174H }}</ref> were used for automated detection of moving objects.


Throughout its tenure, the project was responsible for the discovery of 708 asteroids and one new comet. Of these five were found to be [[near earth asteroid]]s and 8 were [[Mars]]-crossing asteroids.<ref name="ODAS" />
Throughout its tenure, the project observed a total of 10,523 objects, made a total of 44,433 positional measurements, and was responsible for the discovery of 956 asteroids according to the new rules issued by the MPC in October 2010. (The rules redefines who discovered a particular object.<ref name="MPEC 2010-U20" /> Previously, ODAS accounted for a total of 1020 asteroid discoveries). Among the discoveries are also 5 [[near-Earth asteroid]]s and 8 [[Mars-crosser]]s ''(without considering said rule)''. OADS also ''recovered'' several objects that were [[Lost minor planet|previously lost]] and discovered the comet [[198P/ODAS]]<ref name="ODAS" />


== See also ==
== See also ==
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== References ==
== References ==
{{Reflist}}
{{Reflist|refs=

<ref name="ODAS">{{cite web
|last = Hahn
|first = Gerhard
|date = 6 February 2015
|url = http://earn.dlr.de/odas/
|title = O.D.A.S. Home Page
|publisher = European Asteroid Research Node
|accessdate = February 2016}}</ref>

<ref name="Space.com">{{cite web
|last = Paine
|first = Michael
|date = 2000-04-26
|url = http://www.space.com/news/japan_spacewatch_000426.html
|title = Bigger Telescopes Seek Killer Asteroids
|publisher = space.com
|accessdate = 2006-08-13}}</ref>

<ref name="Maury-1998">{{cite conference
|first1 = Alain |last1 = Maury
|first2 = Jean Pierre |last2 = Ragey
|first3 = Hervé |last3 = Viot
|first4 = Harald |last4 = Michaelis
|first5 = Thomas |last5 = Behnke
|date = December 1997
|title = Converting a Schmidt Telescope to CCDs: the OCA/DLR Asteroid Survey
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1998oda..conf..239M
|booktitle = Optical Detectors for Astronomy : Proceedings of an ESO CCD workshop held in Garching, Germany, October 8–10, 1996
|editor = James W. Beletic
|editor2 = Paola Amico
|publisher = Kluwer Academic Publishers
|location = Boston, Mass.
|page = 239
|bibcode = 1998oda..conf..239M
|doi = 10.1007/978-94-011-5262-4_37
|access-date= February 2016}}</ref>

<ref name="Hahn-1998">{{cite journal
|author = Hahn, Gerhard
|date = December 1998
|title = Image processing and astrometric reduction routines of the OCA-DLR Asteroid Survey (O.D.A.S.)
|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1999AcHA....6..174H
|journal = Acta Historica Astronomiae
|page = 174
|bibcode = 1999AcHA....6..174H
|access-date= February 2016}}</ref>

<ref name="MPEC 2010-U20">{{cite web
|title = Minor Planet Electronic Circular – EDITORIAL NOTICE
|work = MPC
|url = http://www.minorplanetcenter.net/mpec/K10/K10U20.html
|date = 19 October 2010}}</ref>
}} <!-- end of reflist -->


[[Category:Astronomical surveys]]
[[Category:Astronomical surveys]]

Revision as of 11:57, 10 February 2016

New Near-Earth
Asteroids Discovered
by O.D.A.S.
  • 1997 NJ6
  • 1997 XV11 recovery
  • 1998 EP8
  • 1998 SJ2
  • 1998 VD31

The OCA-DLR Asteroid Survey (ODAS) was an astronomical survey to search for small Solar System bodies focusing on near-Earth objects in the late 1990s. This European scientific project – a collaboration between the French Observatoire de la Côte d'Azur (OCA) and the German Aerospace Center (DLR) – discovered a total of 956 asteroids and 1 comet during its course.[1]

ODAS operated in cooperation with a global effort regarding Near-Earth objects that was begun by the Working Group on Near-Earth Objects, a component of the International Astronomical Union.[1] The project began October 1996 and ceased observations in April 1999 for a refurbishing. However the telescope has not been reopened since that time.[2] Survey observations were made during the 15 days each month when moon light was at a minimum, during the first and last quarters of the lunar month.[1] The operation used a 90 cm Schmidt telescope of the OCA at Calern, near the city of Nice in southeastern France. A combination of a CCD camera[3] and a software package[4] were used for automated detection of moving objects.

Throughout its tenure, the project observed a total of 10,523 objects, made a total of 44,433 positional measurements, and was responsible for the discovery of 956 asteroids according to the new rules issued by the MPC in October 2010. (The rules redefines who discovered a particular object.[5] Previously, ODAS accounted for a total of 1020 asteroid discoveries). Among the discoveries are also 5 near-Earth asteroids and 8 Mars-crossers (without considering said rule). OADS also recovered several objects that were previously lost and discovered the comet 198P/ODAS[1]

See also

References

  1. ^ a b c d Hahn, Gerhard (6 February 2015). "O.D.A.S. Home Page". European Asteroid Research Node. Retrieved February 2016. {{cite web}}: Check date values in: |accessdate= (help)
  2. ^ Paine, Michael (2000-04-26). "Bigger Telescopes Seek Killer Asteroids". space.com. Retrieved 2006-08-13.
  3. ^ Maury, Alain; Ragey, Jean Pierre; Viot, Hervé; Michaelis, Harald; Behnke, Thomas (December 1997). "Converting a Schmidt Telescope to CCDs: the OCA/DLR Asteroid Survey". In James W. Beletic; Paola Amico (eds.). Optical Detectors for Astronomy : Proceedings of an ESO CCD workshop held in Garching, Germany, October 8–10, 1996. Boston, Mass.: Kluwer Academic Publishers. p. 239. Bibcode:1998oda..conf..239M. doi:10.1007/978-94-011-5262-4_37. Retrieved February 2016. {{cite conference}}: Check date values in: |access-date= (help); Unknown parameter |booktitle= ignored (|book-title= suggested) (help)
  4. ^ Hahn, Gerhard (December 1998). "Image processing and astrometric reduction routines of the OCA-DLR Asteroid Survey (O.D.A.S.)". Acta Historica Astronomiae: 174. Bibcode:1999AcHA....6..174H. Retrieved February 2016. {{cite journal}}: Check date values in: |access-date= (help)
  5. ^ "Minor Planet Electronic Circular – EDITORIAL NOTICE". MPC. 19 October 2010.