Astronomy:907 Rhoda

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Short description: Main-belt asteroid
907 Rhoda
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date12 November 1918
Designations
(907) Rhoda
Pronunciation/ˈroʊdə/[6]
Named afterRhoda Barnard
(wife of E. E. Barnard)[2]
A918 VA · A901 BA
A913 SC · 1918 EU
1913 SC · 1901 BA
Minor planet categorymain-belt [1][3] · (middle)
background [4][5]
Orbital characteristics [3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc118.67 yr (43,343 d)
|{{{apsis}}}|helion}}3.2553 AU
|{{{apsis}}}|helion}}2.3468 AU
2.8010 AU
Eccentricity0.1622
Orbital period4.69 yr (1,712 d)
Mean anomaly183.55°
Mean motion0° 12m 36.72s / day
Inclination19.525°
Longitude of ascending node42.980°
88.326°
Physical characteristics
Mean diameter
  • 62.73±1.7 km[7]
  • 75.22±0.83 km[8]
  • 82.660±0.340 km[9]
Rotation period22.44±0.02 h[10][lower-alpha 1]
Geometric albedo
  • 0.032±0.005[9]
  • 0.040±0.001[8]
  • 0.0560±0.003[7]
  • Tholen = C [3]
  • SMASS = Xk [3]
  • C0 (Barucci)[5]
  • B–V = 0.709±0.020[3]
  • U–B = 0.269±0.029[3]
Absolute magnitude (H)9.7[1][3]


907 Rhoda is a large background asteroid from the central region of the asteroid belt, that measures approximately 75 kilometers (47 miles) in diameter. It was discovered on 12 November 1918, by astronomer Max Wolf at the Heidelberg Observatory in southwest Germany.[1] The dark C/X-type asteroid has a long rotation period of 22.4 hours and is likely spherical in shape. It was named after Rhoda Barnard, wife of American astronomer Edward Emerson Barnard (1857–1923).[2]

Orbit and classification

Rhoda is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.[4][5] It orbits the Sun in the central asteroid belt at a distance of 2.3–3.3 AU once every 4 years and 8 months (1,712 days; semi-major axis of 2.8 AU). Its orbit has an eccentricity of 0.16 and an inclination of 20° with respect to the ecliptic.[3] The body's observation arc begins with its first observation as A901 BA (1901 BA) at the Heidelberg-Königstuhl State Observatory on 18 January 1901, where it was officially discovered almost 18 years later on 12 November 1918.[1]

Naming

This minor planet was named after Rhoda Barnard (née Calvert), wife of the American astronomer Edward Emerson Barnard (1857–1923), who was himself honored with the asteroid 819 Barnardiana. The official naming was published in the journal Astronomische Nachrichten in 1922 (AN 215, 471). The naming was also mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 88).[2]

Physical characteristics

In the Tholen classification, Rhoda is a common, carbonaceous C-type asteroid, while in the Bus–Binzel SMASS classification it is a Xk-subtype, which transitions from the X-type to the uncommon K-type asteroids.[3] In the Barucci-taxonomy, which classified a total of 438 asteroids in 1987, Rhoda is a C0-type.[5]

Rotation period

In April 2004, a rotational lightcurve of Rhoda was obtained from photometric observations by Brian Warner at the Palmer Divide Observatory (716) in Colorado. Lightcurve analysis gave a rotation period of 22.44±0.02 hours with a low brightness variation of 0.16±0.02 magnitude, indicative of a non-elongated, spherical shape ({{{1}}}).[10][lower-alpha 1] Other period determinations were made by Marciniak as well as by Raphaël Nicollerat and Raoul Behrend, giving a low-amplitude lightcurve with a period of 22.46±0.01 and 22.4±0.5 hours, respectively ({{{1}}}).[11][12]

Diameter and albedo

According to the survey carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), Rhoda measures (62.73±1.7), (75.22±0.83) and (82.660±0.340) kilometers in diameter and its surface has an albedo of (0.0560±0.003), (0.040±0.001) and (0.032±0.005), respectively.[7][8][9] The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0560 and calculates a diameter of 62.73 kilometers based on an absolute magnitude of 10.74.[11] Alternative mean-diameter measurements published by the WISE team include in ascending order (67.246±26.594 km), (84.062±30.075 km), (91.045±2.093 km) and (95.22±22.26 km) and albedos of (0.0266±0.0058), (0.03±0.02), (0.031±0.015) and (0.044±0.035).[5][11] An asteroid occultation, observed on 23 March 2009, gave a best-fit ellipse dimension of 63.0 × 63.0 kilometers.[5] These timed observations are taken when the asteroid passes in front of a distant star.[5]

Notes

  1. ↑ 1.0 1.1 Lightcurve plot of (907) Rhoda, Palmer Divide Observatory, B. D. Warner (2004). Rotation period 22.44±0.02 hours with a brightness amplitude of 0.16±0.02 mag. Quality code is 3. Summary figures at the LCDB.

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 "907 Rhoda (A918 VA)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=907. 
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(907) Rhoda". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 81. doi:10.1007/978-3-540-29925-7_908. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 "JPL Small-Body Database Browser: 907 Rhoda (A918 VA)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000907. 
  4. ↑ 4.0 4.1 "Asteroid 907 Rhoda – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=907. 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 "Asteroid 907 Rhoda". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=907+Rhoda. 
  6. ↑ Noah Webster (1884) A Practical Dictionary of the English Language
  7. ↑ 7.0 7.1 7.2 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 24 February 2020. 
  8. ↑ 8.0 8.1 8.2 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)
  9. ↑ 9.0 9.1 9.2 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. 
  10. ↑ 10.0 10.1 Warner, Brian D. (December 2004). "Lightcurve analysis for numbered asteroids 863, 903, 907, 928, 977, 1386 2841, and 75747". Minor Planet Bulletin 31 (4): 85–88. ISSN 1052-8091. Bibcode: 2004MPBu...31...85W. http://www.minorplanet.info/MPB/issues/MPB_31-4.pdf. 
  11. ↑ 11.0 11.1 11.2 "LCDB Data for (907) Rhoda". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=907. 
  12. ↑ Behrend, Raoul. "Asteroids and comets rotation curves – (907) Rhoda". Geneva Observatory. http://obswww.unige.ch/~behrend/page3cou.html#000907. 

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