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827 Wolfiana

From Wikipedia, the free encyclopedia
Florian asteroid

827 Wolfiana
Discovery [1]
Discovered byJ. Palisa
Discovery siteVienna Obs.
Discovery date29 August 1916
Designations
(827) Wolfiana
Named after
Max Wolf[2]
(German astronomer)
1916 ZW · 1928 DK
1940 RA
main-belt · (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc100.68 yr (36,773d)
Aphelion2.6314AU
Perihelion1.9172 AU
2.2743 AU
Eccentricity0.1570
3.43yr (1,253 days)
145.31°
0° 17m 14.64s / day
Inclination3.4231°
172.92°
195.31°
Physical characteristics
Dimensions6.51 km(calculated)[3]
8.488±0.165 km[5]
8.976±0.020 km[6]
4.0±0.3h[7]
4.0654±0.0001 h[8]
0.1153±0.0299[6]
0.129±0.020[5]
0.24(assumed)[3]
S(assumed)[3]
13.1[1][3] · 13.2[6]

827 Wolfiana, provisional designation1916 ZW, is a Florianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered atVienna Observatory on 29 August 1916, by Austrian astronomerJohann Palisa, who named it after German astronomerMax Wolf.[2][9] The assumedstony asteroid has a rotation period of 4.0654 hours.

Orbit and classification

[edit]

Wolfiana is a member of theFlora family (402),[3][4] a giantasteroid family and the largest family of stony asteroids in the main belt.[10]: 23  It orbits the Sun in theinner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,253 days;semi-major axis of 2.27 AU). Its orbit has aneccentricity of 0.16 and aninclination of 3° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Vienna.[9]

Physical characteristics

[edit]

Wolfiana is an assumed stonyS-type asteroid,[3] which agrees with the overallspectral type for Florian asteroids.[10]: 23 

Rotation period

[edit]

In September 2012, a rotationallightcurve ofWolfiana was obtained from photometric observations by American astronomers Luis Martinez, Arizona, andFrederick Pilcher at Organ Mesa Observatory (G50), New Mexico. Lightcurve analysis gave a well-definedrotation period of 4.0654 hours with a brightness amplitude of 0.20magnitude (U=3),[8] refining a period of 4.0 hours previously measured in November 2009 (U=2).[7]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Wolfiana measures 8.488 and 8.976 kilometers in diameter and its surface has analbedo of 0.129 and 0.1153, respectively.[5][6]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 6.51 kilometers based on anabsolute magnitude of 13.1.[3]

Naming

[edit]

Thisminor planet was named by the discoverer in 1920 (AN 211;441) after German astronomer, colleague and friend,Max Wolf (1863–1932), a professor of astronomy atHeidelberg University and founder and director of theHeidelberg-Königstuhl State Observatory, who discovered several novae, comets and 248 minor planets.[2]

The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 82). Asteroid1217 Maximiliana and the lunar craterWolf were also named in his honor.[2]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 827 Wolfiana (1916 ZW)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved12 January 2018.
  2. ^abcdSchmadel, Lutz D. (2007). "(827) Wolfiana".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 76.doi:10.1007/978-3-540-29925-7_828.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (827) Wolfiana". Asteroid Lightcurve Database (LCDB). Retrieved12 January 2018.
  4. ^ab"Asteroid 827 Wolfiana – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  5. ^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.
  6. ^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.
  7. ^abKryszczynska, A.; Colas, F.; Polinska, M.; Hirsch, R.; Ivanova, V.; Apostolovska, G.; et al. (October 2012)."Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region".Astronomy and Astrophysics.546: 51.Bibcode:2012A&A...546A..72K.doi:10.1051/0004-6361/201219199.
  8. ^abPilcher, Frederick; Martinez, Luis (January 2013). "Rotation Period Determination for 827 Wolfiana".The Minor Planet Bulletin.40 (1): 21.Bibcode:2013MPBu...40Q..21P.ISSN 1052-8091.
  9. ^ab"827 Wolfiana (1916 ZW)".Minor Planet Center. Retrieved12 January 2018.
  10. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.

External links

[edit]
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