Astronomy:929 Algunde

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Short description: Main-belt asteroid
929 Algunde
Discovery [1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date10 March 1920
Designations
(929) Algunde
Named afterName picked from the almanac
Lahrer Hinkender Bote [2]
A920 ED · 1920 GR
Minor planet category
Orbital characteristics [3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc99.82 yr (36,460 d)
|{{{apsis}}}|helion}}2.4921 AU
|{{{apsis}}}|helion}}1.9859 AU
2.2390 AU
Eccentricity0.1131
Orbital period3.35 yr (1,224 d)
Mean anomaly249.25°
Mean motion0° 17m 39.12s / day
Inclination3.9128°
Longitude of ascending node231.38°
22.990°
Physical characteristics
Mean diameter
Rotation period3.31016±0.00009 h[9][10]
Geometric albedo
  • 0.242±0.018[7]
  • 0.272±0.072[8]
Absolute magnitude (H)11.7[1][3]


929 Algunde (prov. designation: A920 ED or 1920 GR), is a stony Flora asteroid from the inner regions of the asteroid belt, that measures approximately 11 kilometers (7 miles) in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory on 10 March 1920.[1] The S-type asteroid has a short rotation 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 almanac Lahrer Hinkender Bote.[12]

Orbit and classification

When applying the synthetic hierarchical clustering method (HCM) by Nesvorný,[4] or the 1995 HCM-analysis by Zappalà,[5] Algunde is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the main-belt.[13]:23 However, according to another HCM-analysis by Milani and Knežević (AstDys), it is a background asteroid as this analysis does not recognize the Flora asteroid clan.[6] Algunde orbits the Sun in the inner 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 an eccentricity of 0.11 and an inclination of 4° with respect to the ecliptic.[3] The body's observation arc begins at Heidelberg Observatory on 12 March 1920, two nights after its official discovery observation.[1]

Naming

This minor planet was named "Algunde", after a female name picked from the Lahrer Hinkender Bote, published in Lahr, southern Germany.[2] A Hinkender Bote (lit. "limping messenger") was a very popular almanac,[12] especially in the alemannic-speaking region from the late 17th throughout the early 20th century. The calendar section contains feast days, the dates of important fairs and astronomical ephemerides. For 30 January, the calendar gives "Algunde" as the German name day analogue next to Adelgunde and Martina, the protestant and catholic entries in the calendar of saints, likely referring to Saint Aldegonde and Martina of Rome.[14]

Reinmuth's calendar names

As with 22 other asteroids – starting with 913 Otila, and ending with 1144 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 the Dictionary of Minor Planet Names learned about Reinmuth's source of inspiration from private communications with Dutch astronomer Ingrid van Houten-Groeneveld, who worked as a young astronomer at Heidelberg.[2]

Physical characteristics

In the Tholen classification, Algunde is a common stony S-type asteroid.[3] It is also an S-type in the Bus–DeMeo taxonomy and in the Tholen-like taxonomy of the Small 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 uncommon L-type.[4][11]

Rotation period

In March 2007, a rotational lightcurve of Algunde was obtained from photometric observations by Slovak astronomers Adrián Galád and Leonard Kornoš at Modra Observatory (118). Lightcurve analysis gave a well-defined rotation period of 3.31016±0.00009 hours with a low brightness amplitude of 0.14±0.01 magnitude, indicative of a spherical rather than elongated shape ({{{1}}}).[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

According to the survey carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), Algunde measures (10.70±0.36) and (11.443±0.190) kilometers in diameter and its surface has an albedo of (0.242±0.018) and (0.272±0.072), respectively.[7][8] The Collaborative Asteroid Lightcurve Link takes Petr Pravec's revised WISE data with an albedo of 0.2055 and a diameter of 12.45 kilometers based on an absolute 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

  1. ↑ 1.0 1.1 1.2 1.3 1.4 "929 Algunde (A920 ED)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=929. 
  2. ↑ 2.0 2.1 2.2 Schmadel, 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. https://archive.org/details/dictionaryminorp00schm. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 "JPL Small-Body Database Browser: 929 Algunde (A920 ED)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000929. 
  4. ↑ 4.0 4.1 4.2 4.3 "Asteroid 929 Algunde". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=929+Algunde. 
  5. ↑ 5.0 5.1 Zappalà, V.; Bendjoya, Ph.; Cellino, A.; Farinella, P.; Froeschle, C. (1997). "Asteroid Dynamical Families". NASA Planetary Data System: EAR-A-5-DDR-FAMILY-V4.1. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_5_DDR_FAMILY_V4_1/data/family.tab. Retrieved 15 March 2020. } (PDS main page)
  6. ↑ 6.0 6.1 "Asteroid 929 Algunde – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=929. 
  7. ↑ 7.0 7.1 7.2 Usui, 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  8. ↑ 8.0 8.1 8.2 Masiero, 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. doi:10.1088/0004-637X/791/2/121. Bibcode: 2014ApJ...791..121M. 
  9. ↑ 9.0 9.1 Galad, Adrian; Kornos, Leonard (June 2008). "A Sample of Lightcurves from Modra". The Minor Planet Bulletin 35 (2): 78–81. Bibcode: 2008MPBu...35...78G. http://www.minorplanet.info/MPB/issues/MPB_35-2.pdf. Retrieved 18 February 2020. 
  10. ↑ 10.0 10.1 10.2 10.3 "LCDB Data for (929) Algunde". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=929. 
  11. ↑ 11.0 11.1 11.2 Lazzaro, D.; Angeli, C. A.; Carvano, J. M.; Mothé-Diniz, T.; Duffard, R.; Florczak, M. (November 2004). "S3OS2: the visible spectroscopic survey of 820 asteroids". Icarus 172 (1): 179–220. doi:10.1016/j.icarus.2004.06.006. Bibcode: 2004Icar..172..179L. http://sirrah.troja.mff.cuni.cz/yarko-site/tmp/eos/NEW/spectral_type_figure/s3os2.pdf. Retrieved 18 February 2020. 
  12. ↑ 12.0 12.1 "Lahrer hinkender Bote – Kalender 1925". 1925. p. 1. https://digital.blb-karlsruhe.de/blbihd/periodical/pageview/3467471.  Lahrer Bote archive
  13. ↑ Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV: 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. Bibcode: 2015aste.book..297N. 
  14. ↑ "Lahrer hinkender Bote – Kalender 1925". 1925. p. 6. https://digital.blb-karlsruhe.de/blbihd/periodical/pageview/3467474. 
  15. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (929) Algunde". Geneva Observatory. http://obswww.unige.ch/~behrend/page3cou.html#000929. 

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