Astronomy:838 Seraphina

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838 Seraphina
000838-asteroid shape model (838) Seraphina.png
Shape of Seraphina from modeled lightcurve
Discovery [1]
Discovered byM. F. Wolf
Discovery siteHeidelberg Obs.
Discovery date24 September 1916
Designations
(838) Seraphina
Named afterunknown [2]
A916 SL · 1916 AH
2019 FC5
Minor planet category
Orbital characteristics [3]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc103.28 yr (37,724 d)
|{{{apsis}}}|helion}}3.2777 AU
|{{{apsis}}}|helion}}2.5189 AU
2.8983 AU
Eccentricity0.1309
Orbital period4.93 yr (1,802 d)
Mean anomaly15.248°
Mean motion0° 11m 59.28s / day
Inclination10.423°
Longitude of ascending node240.05°
117.10°
Physical characteristics
Mean diameter
  • 49.36±0.78 km[6]
  • 58.095±0.496 km[7]
  • 59.81±2.3 km[8]
Rotation period15.67±0.02 h[9]
Pole ecliptic latitude(18.0°, 4.0°) (λ1/β1)[10][11]
(192.0°, 32.0°) (λ2/β2)[10][11]
Geometric albedo
  • 0.0455±0.004[8]
  • 0.048±0.008[7]
  • 0.068±0.002[6]
  • Tholen = P [3]
  • X (S3OS2)[12]
  • B–V = 0.703±0.016[3]
  • U–B = 0.324±0.023[3]
Absolute magnitude (H)10.1[1][3]


838 Seraphina (prov. designation: A916 SL or 1916 AH) is a dark and large background asteroid, approximately 58 kilometers (36 miles) in diameter, located in the outer regions of the asteroid belt. It was discovered by German astronomer Max Wolf at the Heidelberg-Königstuhl State Observatory on 24 September 1916.[1] The primitive P-type asteroid has a rotation period of 15.7 hours and is rather spherical in shape. Any reference to the origin of the asteroid's name is unknown.[2]

Orbit and classification

Seraphina 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 outer asteroid belt at a distance of 2.5–3.3 AU once every 4 years and 11 months (1,802 days; semi-major axis of 2.9 AU). Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic.[3] The body's observation arc begins with its official discovery observation at Heidelberg Observatory on 24 September 1916.[1]

Naming

Any reference of this minor planet's name to a person or occurrence is unknown.[2]

Unknown meaning

Among the many thousands of named minor planets, Seraphina is one of 120 asteroids for which no official naming citation has been published. All of these asteroids have low numbers in between 164 Eva and 1514 Ricouxa and were discovered from 1876 up to the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.[13]

Physical characteristics

In the Tholen classification, Seraphina is a very dark, primitive P-type asteroid, that falls into the wider group of the carbonaceous C-Complex.[3] In both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), it is an X-type asteroid.[5][12] P-type asteroids are common in the outer asteroid belt and among the Jupiter trojans.

Rotation period

In November 2005, a rotational lightcurve of Seraphina was obtained from photometric observations by French amateur astronomer Raymond Poncy. Lightcurve analysis gave a rotation period of 15.67±0.02 hours with a low brightness variation of 0.07±0.01 magnitude, indicative of a rather spherical shape ({{{1}}}).[9] Other observations include a period of 16.2 hours with an amplitude of 0.30 magnitude by Richard Binzel from June 1984 ({{{1}}}),[14] and a period of 17.62±0.01 hours with an amplitude of 0.13±0.03 magnitude by the Spanish group of asteroid observers, OBAS, in November 2015 ({{{1}}}).[15]

In 2018, Czech astronomers Josef Ďurech and Josef Hanuš published a modeled lightcurve using photometric data from the Gaia spacecraft's second data release. It showed a sidereal period of 11.7245±0.0002 hours ({{{1}}}), and gave two spin axes at (18.0°, 4.0°) and (192.0°, 32.0°) in ecliptic coordinates (λ, β).[10][11]

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite, the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer (WISE), and the Infrared Astronomical Satellite IRAS, Seraphina measures (49.36±0.78), (58.095±0.496) and (59.81±2.3) kilometers in diameter and its surface has an albedo of (0.068±0.002), (0.048±0.008) and (0.0455±0.004), respectively.[6][7][8] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0427 and a diameter of 59.75 kilometers based on an absolute magnitude of 10.16.[11] Alternative mean-diameter measurements published by the WISE team include (43.24±13.99 km), (48.861±11.16 km) and (65.33±0.24 km) with corresponding albedos of (0.04), (0.062±0.081) and (0.0820±0.0418).[5][11]

Two asteroid occultations of Seraphina gave a best-fit ellipse dimension of (60.0 km × 60.0 km) and (49.0 km × 49.0 km) for their respective observation on 5 February 2007 and on 20 July 2014. These timed observations are taken when the asteroid passes in front of a distant star. However, these two observations have received a poor quality rating.[5]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 Cite error: Invalid <ref> tag; no text was provided for refs named MPC-object
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(838) Seraphina". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 77. doi:10.1007/978-3-540-29925-7_839. ISBN 978-3-540-00238-3. https://archive.org/details/dictionaryminorp00schm. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 "JPL Small-Body Database Browser: 838 Seraphina (A916 SL)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000838. 
  4. ↑ 4.0 4.1 "Asteroid 838 Seraphina – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=838. 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 "Asteroid 838 Seraphina". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=838+Seraphina. 
  6. ↑ 6.0 6.1 6.2 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)
  7. ↑ 7.0 7.1 7.2 Mainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R. et al. (June 2016). "NEOWISE Diameters and Albedos V1.0". NASA Planetary Data System. Bibcode: 2016PDSS..247.....M. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab. Retrieved 8 March 2020. 
  8. ↑ 8.0 8.1 8.2 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 8 March 2020. 
  9. ↑ 9.0 9.1 Behrend, Raoul. "Asteroids and comets rotation curves – (838) Seraphina". Geneva Observatory. http://obswww.unige.ch/~behrend/page3cou.html#000838. 
  10. ↑ 10.0 10.1 10.2 Ďurech, J.; Hanuš, J. (November 2018). "Reconstruction of asteroid spin states from Gaia DR2 photometry". Astronomy and Astrophysics 620: A91. doi:10.1051/0004-6361/201834007. ISSN 0004-6361. Bibcode: 2018A&A...620A..91D. 
  11. ↑ 11.0 11.1 11.2 11.3 11.4 "LCDB Data for (838) Seraphina". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=838. 
  12. ↑ 12.0 12.1 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 8 March 2020. 
  13. ↑ Cite error: Invalid <ref> tag; no text was provided for refs named DOMPN-unknown
  14. ↑ Binzel, R. P. (October 1987). "A photoelectric survey of 130 asteroids". Icarus 72 (1): 135–208. doi:10.1016/0019-1035(87)90125-4. ISSN 0019-1035. Bibcode: 1987Icar...72..135B. 
  15. ↑ Aznar Macias, Amadeo; Carreno Garcerain, Alfonso; Arce Mansego, Enrique; Brines Rodriguez, Pedro; Lozano de Haro, Juan; Fornas Silva, Alvaro et al. (April 2016). "Twenty-three Asteroids Lightcurves at Observadores de Asteroides (OBAS): 2015 October - December". Minor Planet Bulletin 43 (2): 174–181. ISSN 1052-8091. Bibcode: 2016MPBu...43..174A. http://www.minorplanet.info/MPB/issues/MPB_43-2.pdf. Retrieved 8 March 2020. 

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