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7655 Adamries

From Wikipedia, the free encyclopedia
Not to be confused with236305 Adamriess.

7655 Adamries
Discovery [1]
Discovered byF. Börngen
Discovery siteKarl Schwarzschild Obs.
Discovery date28 December 1991
Designations
(7655) Adamries
Named after
Adam Ries
(mathematician)[2]
1991 YM1 · 1977 BW
main-belt · Nysa[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc39.60 yr (14,464 days)
Aphelion2.7494AU
Perihelion2.0848 AU
2.4171 AU
Eccentricity0.1375
3.76yr (1,373 days)
289.57°
0° 15m 44.28s / day
Inclination4.0156°
103.41°
8.9941°
Physical characteristics
Dimensions3.60 km(calculated)[3]
4.21±0.96 km[4]
22.8758±0.1133h[5]
0.21(assumed)[3]
0.250±0.124[4]
C[6] · S[3]
14.00[4] · 14.081±0.004(R)[5] · 14.1[1] · 14.53[3] · 14.56±0.26[6]

7655 Adamries, provisional designation1991 YM1, is a Nysaasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter. It was discovered on 28 December 1991, by German astronomerFreimut Börngen atKarl Schwarzschild Observatory in Tautenburg, eastern Germany.[7] It was named after mathematicianAdam Ries.[2]

Classification and orbit

[edit]

Adamries is a member of theNysa family, one of the prominent families of theinner main-belt, named after its namesake44 Nysa. It orbits the Sun at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,373 days). Its orbit has aneccentricity of 0.14 and aninclination of 4° with respect to theecliptic.[1]Adamries was first identified as1977 BW atCrAO/Nauchnyj in 1977, extending the asteroid'sobservation arc by 15 years prior to its official discovery observation.[7]

Physical characteristics

[edit]

Adamries has been characterized as a carbonaceousC-type asteroid byPan-STARRS' photometric survey.[6] It is also an assumed stonyS-type asteroid.[3]

Lightcurve

[edit]

In September 2013, rotationallightcurve ofAdamries was obtained from photometric observation by astronomers at thePalomar Transient Factory in California. It showed a longer-than-averagerotation period of22.8758 hours with a brightness variation of 0.33magnitude (U=2).[5]

Diameter and albedo

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According to the survey carried out by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Adamries measures 4.2 kilometers in diameter and its surface has analbedo of 0.25, which is typical for stony asteroids.[4] CALL assumes a standard albedo for stony asteroids of 0.21 and calculates a diameter of 3.6 kilometers with anabsolute magnitude of 14.53.[3]

Naming

[edit]

Thisminor planet was named in honor of famous German mathematicianAdam Ries (1492–1559), who wrote the first Germanarithmetic book in the 16th century, explaining in simple terms to the common people how to do arithmetic.[2]

At the time, this was considered to be difficult. This minor planet was the100th numbered discovery of astronomer Freimut Börngen.[2] The approved naming citation was published by theMinor Planet Center on 18 August 1997(M.P.C. 30478).[8] This minor planet should not be confused with236305 Adamriess, named after American astronomer and 2011 Nobel Prize winnerAdam Riess.

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 7655 Adamries (1991 YM1)" (2016-08-27 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(7655) Adamries".Dictionary of Minor Planet Names – (7655) Adamries.Springer Berlin Heidelberg. p. 608.doi:10.1007/978-3-540-29925-7_6601.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (7655) Adamries". Asteroid Lightcurve Database (LCDB). Retrieved29 April 2016.
  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. Retrieved29 April 2016.
  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. Retrieved29 April 2016.
  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. Retrieved29 April 2016.
  7. ^ab"7655 Adamries (1991 YM1)".Minor Planet Center. Retrieved29 April 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 April 2016.

External links

[edit]
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