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4756 Asaramas

From Wikipedia, the free encyclopedia
Minor planet

4756 Asaramas
Discovery[1]
Discovered byLa Plata Obs.
Discovery siteLa Plata Obs.
Discovery date21 April 1950
Designations
(4756) Asaramas
Named after
Asociación Argentina Amigos de la Astronomía
(astronomical association)[2]
1950 HJ · 1976 FD
1983 RH9
main-belt · Eos[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.94 yr (24,449 days)
Aphelion3.2128AU
Perihelion2.8233 AU
3.0180 AU
Eccentricity0.0645
5.24yr (1,915 days)
262.30°
0° 11m 16.8s / day
Inclination9.2037°
239.42°
2.4305°
Physical characteristics
Dimensions10.78 km(calculated)[3]
11.644±0.215 km[4]
16.536±0.0087h[5]
0.14(assumed)[3]
0.188±0.025[4]
L[6] · S[3]
11.78±0.06[6] · 12.10[4] · 12.140±0.002(R)[5] · 12.2[1] · 12.59[3]

4756 Asaramas, provisional designation1950 HJ, is a stony rare-type Eoanasteroid from the outer region of theasteroid belt, approximately 11 kilometers in diameter. It was discovered on 21 April 1950, by astronomers at theLa Plata Astronomical Observatory in Argentina.[7] It is named for the astronomical societyAsociación Argentina Amigos de la Astronomía.[2]

Classification and orbit

[edit]

Asaramas is a member of theEos family (606), the largestasteroid family in theouter main belt consisting of nearly 10,000 asteroids. It orbits the Sun at a distance of 2.8–3.2 AU once every 5 years and 3 months (1,915 days). Its orbit has aneccentricity of 0.06 and aninclination of 9° with respect to theecliptic.[1]

As noprecoveries were taken and no prior identifications were made, the body'sobservation arc begins with its official discovery observation at La Plata.[7]

Physical characteristics

[edit]

Asaramas has been characterized as aL-type asteroid byPanSTARRS' photometric survey.[6]

Rotation period

[edit]

In November 2010, a rotationallightcurve ofAsaramas was obtained from photometric observations in the R-band at thePalomar Transient Factory in California. Lightcurve analysis gave a typicalrotation period of 16.536 hours with a brightness variation of 0.16magnitude (U=2).[5]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Asaramas measures 11.64 kilometers in diameter and its surface has analbedo of 0.188,[4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for Eoan asteroids of 0.14 and calculates a diameter of 10.78 kilometers, based on anabsolute magnitude of 12.59.[3]

Naming

[edit]

Thisminor planet was named in honor of theAsociación Argentina Amigos de la Astronomía (A.A.A.A or Asaramas), an astronomical society for amateur astronomers in Argentina. Founded on 4 January 1929, the A.A.A.A. was the first contact with astronomy for a large number of professional astronomers at the La Plata Observatory.[2] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22503).[8]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4756 Asaramas (1950 HJ)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 8 March 2017. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4756) Asaramas".Dictionary of Minor Planet Names – (4756) Asaramas.Springer Berlin Heidelberg. p. 409.doi:10.1007/978-3-540-29925-7_4663.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4756) Asaramas". Asteroid Lightcurve Database (LCDB). Retrieved7 March 2017.
  4. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved7 March 2017.
  5. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved7 March 2017.
  6. ^abcVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved7 March 2017.
  7. ^ab"4756 Asaramas (1950 HJ)".Minor Planet Center. Retrieved7 March 2017.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 March 2017.

External links

[edit]
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