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3905 Doppler

From Wikipedia, the free encyclopedia
Main belt asteroid

3905 Doppler
Discovery[1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date28 August 1984
Designations
(3905) Doppler
Pronunciation/ˈdɒplər/[2]
Named after
Christian Doppler
(Austrian physicist)[3]
1984 QO · 1980 RP2
main-belt
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc35.81 yr (13,078 days)
Aphelion3.2190AU
Perihelion1.9001 AU
2.5596 AU
Eccentricity0.2577
4.10yr (1,496 days)
320.23°
0° 14m 26.52s / day
Inclination14.192°
343.32°
90.823°
Knownsatellites1[4][5]
Physical characteristics
Dimensions8.021±0.047 km[6]
50.8±0.1h[5]
0.228±0.040[6]
S[5]
12.6[1][5]

3905 Doppler, provisional designation1984 QO, is a stonyasteroid andbinary system from the middle region of theasteroid belt, approximately 8 kilometers in diameter.

The asteroid was discovered on 28 August 1984, by Czech astronomerAntonín Mrkos atKleť Observatory and named after physicistChristian Doppler.[3][7]

Orbit and characterization

[edit]

Doppler orbits the Sun in thecentral main-belt at a distance of 1.9–3.2 AU once every 4 years and 1 month (1,496 days). Its orbit has aneccentricity of 0.26 and aninclination of 14° with respect to theecliptic.[1] It has been characterized as a commonS-type asteroid.[5]

Aminor-planet moon orbitingDoppler every 50.8 hours (or 2 days, 2 hours, and 48 minutes) was found orbiting the asteroid in 2013. This is fairly longorbital period for a moon of an asteroid of this size.[4] The satellite's orbital period is identical to the primary'srotation period (F-type binary).[5]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Doppler measures 8.021 kilometers in diameter and its surface has analbedo of 0.228,[6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.97 kilometers with anabsolute magnitude of 12.6.[5]

Naming

[edit]

Thisminor planet was named afterChristian Doppler (1803–1853), Austrian physicist in Vienna and well known for theDoppler effect, which he first described in 1842, in his book "Ueber das farbige Licht der Doppelsterne". The naming was proposed byJana Tichá and M. Šolc.[3] The approved naming citation was published by theMinor Planet Center on 28 August 1996 (M.P.C. 27734).[8]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 3905 Doppler (1984 QO)" (2016-06-29 last obs.).Jet Propulsion Laboratory. Retrieved15 June 2017.
  2. ^"Doppler".Dictionary.com Unabridged (Online). n.d.
  3. ^abcSchmadel, Lutz D. (2007). "(3905) Doppler".Dictionary of Minor Planet Names – (3905) Doppler.Springer Berlin Heidelberg. p. 332.doi:10.1007/978-3-540-29925-7_3894.ISBN 978-3-540-00238-3.
  4. ^abJohnston, Robert (21 September 2014)."(3905) Doppler". johnstonsarchive.net. Retrieved15 June 2017.
  5. ^abcdefg"LCDB Data for (3905) Doppler". Asteroid Lightcurve Database (LCDB). Retrieved15 June 2017.
  6. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved15 June 2017.
  7. ^"3905 Doppler (1984 QO)".Minor Planet Center. Retrieved15 June 2017.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 June 2017.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
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Authority control databasesEdit this at Wikidata
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