1001 Gaussia
U–B = 0.265[1] | |
9.70[4][5][11] · 9.72[6] · 9.77[7][9][10] · 9.8[1] · 9.91±0.26[14] | |
Gaussia (
Orbit and classification
Gaussia is a background asteroid that does not belong to any known asteroid family. It orbits the Sun in the outer main-belt at a distance of 2.8–3.6 AU once every 5 years and 9 months (2,100 days). Its orbit has an eccentricity of 0.13 and an inclination of 9° with respect to the ecliptic.[1]
The asteroid was first identified as A907 XC at Taunton Observatory (
Physical characteristics
In the
Rotation period
In November 2005, a rotational
Lower-rated lightcurves with a divergent period of 4.08 and 9.17 hours were previously obtained in 2005 and 2009, respectively (
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0417 and a diameter of 74.71 kilometers based on an absolute magnitude of 9.7.[4]
Naming
This
The official naming citation was mentioned in
1001 Gaussia was named as part of trio honoring the events surrounding the discovery of Ceres in 1801.[17] Carl Friedrich Gauss who computed the orbit of Ceres was for 1001 Gaussia, 1000 Piazzia for Giuseppe Piazzi and 1002 Olbersia for Heinrich Wilhelm Matthias Olbers.[17] Olbers recovered Ceres after it has passed behind the Sun and returned.[17] In the next few years only three more astronomical bodies were found between Mars and Jupiter, Pallas, Juno, and 4 Vesta, however it would be 37 years before another asteroid was found, 5 Astraea in 1845.[17]
Notes
- ^ a b Aznar (2016a): Observation 2015-11-22. Rotation period 20.99±0.01 hours with a brightness amplitude of 0.11±0.01 mag. Quality Code of 3. Summary figures for (1001) Gaussia at Collaborative Asteroid Lightcurve Link (CALL)
See also
References
- ^ a b c d e f g h i "JPL Small-Body Database Browser: 1001 Gaussia (1923 OA)" (2017-05-01 last obs.). Jet Propulsion Laboratory. Retrieved 5 September 2017.
- ^ "Gaussian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ ISBN 978-3-540-00238-3.
- ^ a b c d e f g "LCDB Data for (1001) Gaussia". Asteroid Lightcurve Database (LCDB). Retrieved 5 September 2017.
- ^ S2CID 9341381.
- ^ S2CID 119289027.
- ^ S2CID 118700974.
- ^ S2CID 119293330.
- ^ Bibcode:2004PDSS...12.....T. Retrieved 22 October 2019.
- ^ )
- ^ S2CID 46350317.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1001) Gaussia". Geneva Observatory. Retrieved 5 September 2017.
- ^ ISSN 1052-8091.
- S2CID 53493339.
- ^ a b "1001 Gaussia (1923 OA)". Minor Planet Center. Retrieved 5 September 2017.
- Bibcode:1941ASPL....3..365N.
- ^ Bibcode:1941ASPL....3..365N.
External links
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 1001 Gaussia at AstDyS-2, Asteroids—Dynamic Site
- 1001 Gaussia at the JPL Small-Body Database