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1726 Hoffmeister

From Wikipedia, the free encyclopedia
Asteroid

1726 Hoffmeister
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date24 July 1933
Designations
(1726) Hoffmeister
Named after
Cuno Hoffmeister
(German astronomer)[2]
1933 OE · 1955 FC
1955 HX · 1957 WD
A924 UA
main-belt · (middle)
Hoffmeister[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc91.85 yr (33,547 days)
Aphelion2.9051AU
Perihelion2.6702 AU
2.7877 AU
Eccentricity0.0421
4.65yr (1,700 days)
42.063°
0° 12m 42.48s / day
Inclination3.4833°
230.97°
69.026°
Physical characteristics
Dimensions17.35 km(calculated)[5]
22.03±5.39[6]
22.52±0.23 km[7]
24.61±0.52[8]
25.250±0.079 km[9]
25.438±0.118 km[10]
25.67±8.37[11]
11.7058±0.0056h[12]
0.03±0.03[11]
0.0360±0.0066[10]
0.037±0.005[9]
0.042±0.006[7]
0.044±0.002[8]
0.05±0.05[6]
0.057(assumed)[5]
SMASS = Cb[1] · C[5][13]
12.082±0.002(R)[12] · 12.10[8] · 12.26[11] · 12.2[10] · 12.3[1][6][7] · 12.53[5] · 12.54±0.24[13]

1726 Hoffmeister, provisional designation1933 OE, is a carbonaceousasteroid and namesake of theHoffmeister family from the central region of theasteroid belt, approximately 23 kilometers in diameter.

It was discovered on 24 July 1933, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany, and named after astronomerCuno Hoffmeister.[14]

Orbit and classification

[edit]

Hoffmeister is the namesake and lowest-numbered member of the very compactHoffmeister family (519), which, based upon its low albedo, was most likely formed from the breakup of a 50–100 kilometer-sized, carbon-richparent body within the past several hundred million years.[3][4]

It orbits the Sun in thecentral main-belt at a distance of 2.7–2.9 AU once every 4 years and 8 months (1,700 days;semi-major axis of 2.79 AU). Its orbit has aneccentricity of 0.04 and aninclination of 3° with respect to theecliptic.[1] It was first identified as1924 UA at theYerkes Observatory in 1924, extending the asteroid'sobservation arc by 9 years prior to its official discovery observation at Heidelberg.[14]

Physical characteristics

[edit]

In theSMASS classification,Hoffmeister is characterized as a Cb-type, a subtype of the carbonaceousC-complex.[1][13]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Hoffmeister measures between 22.03 and 25.67 kilometers in diameter, and its surface has a lowalbedo between 0.03 and 0.05.[6][7][8][9][10][11] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 17.4 kilometers with anabsolute magnitude of 12.53.[5]

Rotational lightcurve

[edit]

In December 2009, a rotationallightcurve ofHoffmeister was obtained from photometric observations by astronomers at thePalomar Transient Factory in California. It gave arotation period of11.7058±0.0056 hours with a brightness variation of 0.40magnitude (U=2).[12]

Naming

[edit]

Thisminor planet was named in memory of German astronomerCuno Hoffmeister (1892–1968), who founded theSonneberg Observatory in 1925, and became one of its directors(see1039 Sonneberga). Hoffmeister discovered thousands ofvariable stars, co-discovered cometC/1959 O1, thoroughly investigated a large number ofmeteors, and discovered 5 minor planets:2183 Neufang,3203 Huth,3674 Erbisbühl,4183 Cuno (which was later named after him) and4724 Brocken. The lunar craterHoffmeister was also named in his honor.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3933).[15]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1726 Hoffmeister (1933 OE)" (2016-08-27 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 August 2020. Retrieved1 July 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1726) Hoffmeister".Dictionary of Minor Planet Names – (1726) Hoffmeister.Springer Berlin Heidelberg. p. 137.doi:10.1007/978-3-540-29925-7_1727.ISBN 978-3-540-00238-3.
  3. ^abMigliorini, F.; Manara, A.; di Martino, M.; Farinella, P. (June 1996)."The Hoffmeister asteroid family: inferences from physical data".Astronomy and Astrophysics.310:681–685.Bibcode:1996A&A...310..681M. Retrieved17 November 2015.
  4. ^abCarruba, V.; Novakovic, B.; Aljbaae, S. (March 2017)."The Hoffmeister asteroid family".Monthly Notices of the Royal Astronomical Society.465 (4):4099–4105.arXiv:1611.06176.Bibcode:2017MNRAS.465.4099C.doi:10.1093/mnras/stw3022.
  5. ^abcde"LCDB Data for (1726) Hoffmeister". Asteroid Lightcurve Database (LCDB). Retrieved28 October 2016.
  6. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved19 April 2017.
  7. ^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.S2CID 46350317. Retrieved28 October 2016.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  9. ^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.S2CID 119293330. Retrieved28 October 2016.
  10. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.S2CID 35447010.
  11. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  12. ^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.S2CID 8342929. Retrieved28 October 2016.
  13. ^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.S2CID 53493339. Retrieved28 October 2016.
  14. ^ab"1726 Hoffmeister (1933 OE)".Minor Planet Center. Retrieved28 October 2016.
  15. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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