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929 Algunde

From Wikipedia, the free encyclopedia
Main-belt asteroid

929 Algunde
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date10 March 1920
Designations
(929) Algunde
Named after
Name picked from the almanac
Lahrer Hinkender Bote[2]
A920 ED · 1920 GR
Orbital characteristics[3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc99.82yr (36,460 d)
Aphelion2.4921AU
Perihelion1.9859 AU
2.2390 AU
Eccentricity0.1131
3.35 yr (1,224 d)
249.25°
0° 17m 39.12s / day
Inclination3.9128°
231.38°
22.990°
Physical characteristics
3.31016±0.00009 h[9][10]
  • 0.242±0.018[7]
  • 0.272±0.072[8]
11.7[1][3]

929 Algunde (prov. designation:A920 EDor1920 GR), is a stonyFlora asteroid from the inner regions of theasteroid belt, that measures approximately 11 kilometers (7 miles) in diameter. It was discovered by German astronomerKarl Reinmuth at theHeidelberg-Königstuhl State Observatory on 10 March 1920.[1] TheS-type asteroid has a shortrotation period of 3.3 hours and is likely spherical in shape. It was named "Algunde", a common German female name unrelated to the discoverer's contemporaries, that was taken from the almanacLahrer Hinkender Bote.[12]

Orbit and classification

[edit]

When applying the synthetichierarchical clustering method (HCM) byNesvorný,[4] or the 1995 HCM-analysis byZappalà,[5]Algunde is a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[13]: 23  However, according to another HCM-analysis byMilani andKnežević (AstDys), it is abackground asteroid as this analysis does not recognize the Floraasteroid clan.[6]Algunde orbits the Sun in theinner asteroid belt at a distance of 2.0–2.5 AU once every 3 years and 4 months (1,224 days;semi-major axis of 2.24 AU). Its orbit has aneccentricity of 0.11 and aninclination of 4° with respect to theecliptic.[3] The body'sobservation arc begins atHeidelberg Observatory on 12 March 1920, two nights after its official discovery observation.[1]

Naming

[edit]

Thisminor planet was named "Algunde", after a female name picked from theLahrer Hinkender Bote, published inLahr, southern Germany.[2] AHinkender Bote (lit. "limping messenger") was a very popularalmanac,[12] especially in thealemannic-speaking region from the late 17th throughout the early 20th century. Thecalendar section containsfeast days, the dates of important fairs andastronomical ephemerides. For 30 January, the calendar gives "Algunde" as the Germanname day analogue next toAdelgunde andMartina, the protestant and catholic entries in thecalendar of saints, likely referring to SaintAldegonde andMartina of Rome.[14]

Reinmuth'scalendar names

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As with 22 other asteroids – starting with913 Otila, and ending with1144 Oda – Reinmuth selected names from this calendar due to his many asteroid discoveries that he had trouble thinking of proper names. These names are not related to the discoverer's contemporaries.Lutz Schmadel, the author of theDictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomerIngrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]

Physical characteristics

[edit]

In theTholen classification,Algunde is a common stonyS-type asteroid.[3] It is also an S-type in theBus–DeMeo taxonomy and in the Tholen-like taxonomy of theSmall Solar System Objects Spectroscopic Survey (S3OS2). Only in the SMASS-like taxonomy of the S3OS2,Algunde is an Sl-subtype asteroid that transitions between the S-type and the uncommonL-type.[4][11]

Rotation period

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In March 2007, a rotationallightcurve ofAlgunde was obtained fromphotometric observations by Slovak astronomersAdrián Galád andLeonard Kornoš atModra Observatory (118). Lightcurve analysis gave a well-definedrotation period of3.31016±0.00009 hours with a low brightness amplitude of0.14±0.01magnitude, indicative of a spherical rather than elongated shape (U=3).[9] Between 2008 and 2018, numerous follow-up observations by other astronomers confirmed the period of 3.31 hours with brightness variation maxima between 0.11 and 0.17.[10][15]

Diameter and albedo

[edit]

According to the survey carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer (WISE),Algunde measures (10.70±0.36) and (11.443±0.190) kilometers in diameter and its surface has analbedo of (0.242±0.018) and (0.272±0.072), respectively.[7][8] TheCollaborative Asteroid Lightcurve Link takesPetr Pravec's revised WISE data with an albedo of 0.2055 and a diameter of 12.45 kilometers based on anabsolute magnitude of 11.86.[10] Another publication by the WISE team gives a mean-diameter of (12.440±0.073) kilometers and an albedo of (0.2348±0.0327).[10]

References

[edit]
  1. ^abcde"929 Algunde (A920 ED)".Minor Planet Center. Retrieved18 February 2020.
  2. ^abcSchmadel, Lutz D. (2007). "(929) Algunde".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 82.doi:10.1007/978-3-540-29925-7_930.ISBN 978-3-540-00238-3.
  3. ^abcdef"JPL Small-Body Database Browser: 929 Algunde (A920 ED)" (2020-01-05 last obs.).Jet Propulsion Laboratory. Retrieved18 February 2020.
  4. ^abcd"Asteroid 929 Algunde".Small Bodies Data Ferret. Retrieved18 February 2020.
  5. ^abZappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997)."Asteroid Dynamical Families".NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. Retrieved15 March 2020. (PDS main page)
  6. ^ab"Asteroid 929 Algunde – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved18 February 2020.
  7. ^abcUsui, 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)
  8. ^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.
  9. ^abGalad, Adrian; Kornos, Leonard (June 2008)."A Sample of Lightcurves from Modra"(PDF).The Minor Planet Bulletin.35 (2):78–81.Bibcode:2008MPBu...35...78G. Archived fromthe original(PDF) on 13 February 2020. Retrieved18 February 2020.
  10. ^abcd"LCDB Data for (929) Algunde". Asteroid Lightcurve Database (LCDB). Retrieved18 February 2020.
  11. ^abcLazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004)."S3OS2: the visible spectroscopic survey of 820 asteroids"(PDF).Icarus.172 (1):179–220.Bibcode:2004Icar..172..179L.doi:10.1016/j.icarus.2004.06.006. Retrieved18 February 2020.
  12. ^ab"Lahrer hinkender Bote – Kalender 1925".Badischen Landesbibliothek. 1925. p. 1. Retrieved18 February 2020.Lahrer Bote archive
  13. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV:297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.
  14. ^"Lahrer hinkender Bote – Kalender 1925".Badischen Landesbibliothek. 1925. p. 6. Retrieved18 February 2020.
  15. ^Behrend, Raoul."Asteroids and comets rotation curves – (929) Algunde".Geneva Observatory. Retrieved18 February 2020.

External links

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