Astronomy:1313 Berna

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Short description: Asteroid
1313 Berna
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date24 August 1933
Designations
(1313) Berna
Named afterBern[2]
(capital of Switzerland)
1933 QG · 1926 EA
A911 OA
Minor planet categorymain-belt[1][3] · (middle)
background[4][5]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc84.74 yr (30,953 d)
|{{{apsis}}}|helion}}3.2074 AU
|{{{apsis}}}|helion}}2.1112 AU
2.6593 AU
Eccentricity0.2061
Orbital period4.34 yr (1,584 d)
Mean anomaly241.65°
Mean motion0° 13m 38.28s / day
Inclination12.545°
Longitude of ascending node298.14°
99.773°
Known satellites1(see 2nd infobox)[lower-alpha 1]
Physical characteristics
Mean diameter13.12±2.44 km[6]
13.504±0.311 km[7][8][9]
13.93±0.64 km[10]
14.27±0.36 km[11]
19.96±4.97 km[12]
Mass(2.25±2.00)×1015 kg[10]
Mean density1.21±0.14 cm3[10]
Rotation period25.46 h[13][14][15][16]
Geometric albedo0.13[12]
0.169[11]
0.185[7][8][9]
0.212[17]
0.245[6]
S (assumed)[13]
Absolute magnitude (H)11.55[6]
11.6[1][3][13]
11.69±0.12[17]
11.75[12]
11.80[7][9][11]


1313 Berna, provisional designation 1933 QG, is a background asteroid and synchronous binary system from the Eunomian region in the central asteroid belt, approximately 14 kilometers (8.7 miles) in diameter. It was discovered on 24 August 1933, by Belgian astronomer Sylvain Arend at the Uccle Observatory in Belgium.[1] The assumed S-type asteroid has a longer-than average rotation period of 25.5 hours and is likely elongated in shape.[13] It was named for the Swiss capital of Bern.[1] The discovery of an 11-kilometer-sized companion was announced in February 2004.[lower-alpha 1]

Orbit and classification

According to modern HCM-analyses by Nesvorný, as well as by Milani and Knežević, Berna is a non-family asteroid from the main belt's background population.[4][5]

Based on osculating Keplerian orbital elements, it is located in the region of the Eunomia family (502), a prominent family of stony asteroids.[13] It orbits the Sun in the central asteroid belt at a distance of 2.1–3.2 AU once every 4 years and 4 months (1,584 days; semi-major axis of 2.66 AU). Its orbit has an eccentricity of 0.21 and an inclination of 13° with respect to the ecliptic.[3] In 1911, Berna was first identified as A911 OA at Johannesburg. Its observation arc begins with its official discovery observation at Uccle.[1]

Naming

This minor planet was named after the Swiss capital city of Bern. The name was proposed by Sigmund Mauderli (1876–1962), astronomer and director of the Astronomical Institute at the University of Bern, after whom 1748 Mauderli is named. He computed the definitive orbit of the body, and also insisted to rename the minor planet to its current name, after it had been originally published as "Bernia".[2] The official naming citation was first mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 120).[2]

Physical characteristics

S/2004 (1313) 1
Discovery[lower-alpha 1]
Discovered byR. Behrend, R. Roy
S. Sposetti
Discovery date6 February 2004
Light-curve
Orbital characteristics
25 km
Orbital period25.464±0.001 h[17][14]
Angular distance30 mas (maximum)
Satellite of1313 Berna
Physical characteristics
Dimensions8.37 km[18]
Apparent magnitudeΔ0.51 fainter than prim.
Absolute magnitude (H)12.8–13.0


Lightcurve

A network of astronomers at several observatories including Raoul Behrend at Geneva Observatory, Switzerland, obtained the so-far best rated rotational light-curve of Berna. Light-curve analysis gave a rotation period of 25.464 hours with a brightness variation of 0.28 magnitude ({{{1}}}).[15] In November 2007, photometric observations at Cerro Tololo, Chile, using its 0.9-meter Prompt5 telescope in combination with the Spitzer Space Telescope gave a concurring period of 25.46 hours with an amplitude of 0.5 magnitude ({{{1}}}).[17]:40 Other light-curves were also obtained by several amateur astronomers giving a period of 6, 25.4 and 25.45 hours, respectively ({{{1}}}).[16]

Asteroid moon

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite, NASA's Spitzer Space Telescope and the Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Berna measures between 13.12 and 19.96 kilometers in diameter and its surface has an albedo between 0.13 and 0.25.[6][17][9][8][11][12] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from 15 Eunomia, the parent body of the Eunomia family – and calculates a diameter of 13.88 kilometers based on an absolute magnitude of 11.6.[13]

Notes

  1. ↑ 1.0 1.1 1.2 International Astronomical Union Circular (No.8292), 23 February 2004 for (1313) BERNA:

    "Photometric observations obtained of the minor planet (1313) on eight nights during Feb. 6–16 show a lightcurve amplitude of 0.25 magnitude and suggest that this is a binary system with an orbital period of 1.061 ± 0.005 days, showing mutual eclipses and/or occultations near both rotational lightcurve minima with a duration of about 0.09 day and depth about 0.7 mag, the first being centered on Feb. 7.85 UT. The regular-appearing lightcurve is synchronized with the eclipse events, indicating that at least one of the two bodies is elongated and rotates synchronously with the orbital motion; the sharp eclipse/occultation events indicate that both components have approximately the same size. The maximum orbital separation observed from earth would be about 0".03."

    — Reported by R. Behrend, Geneva Observatory, on behalf of R. Roy, S. Sposetti, N. Waelchli, D. Pray, N. Berger, C. Demeautis, D.Matter, R. Durkee, A. Klotz, D. Starkey, and V. Cotrez)

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 "1313 Berna (1933 QG)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1313. 
  2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(1313) Berna". Dictionary of Minor Planet Names – (1313) Berna. Springer Berlin Heidelberg. p. 107. doi:10.1007/978-3-540-29925-7_1314. ISBN 978-3-540-00238-3. 
  3. ↑ 3.0 3.1 3.2 3.3 "JPL Small-Body Database Browser: 1313 Berna (1933 QG)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001313. 
  4. ↑ 4.0 4.1 "Asteroid 1313 Berna". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1313+Berna. 
  5. ↑ 5.0 5.1 "Asteroid (1313) Berna – Proper elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?n=1313&pc=1.1.6. 
  6. ↑ 6.0 6.1 6.2 6.3 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C. et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters 759 (1): 5. doi:10.1088/2041-8205/759/1/L8. Bibcode: 2012ApJ...759L...8M. 
  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: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0. Bibcode: 2016PDSS..247.....M. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_COMPIL_5_NEOWISEDIAM_V1_0/data/neowise_mainbelt.tab. Retrieved 11 December 2018. 
  8. ↑ 8.0 8.1 8.2 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J. et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal 741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. 
  9. ↑ 9.0 9.1 9.2 9.3 Mainzer, 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M.  (catalog)
  10. ↑ 10.0 10.1 10.2 Carry, B. (December 2012). "Density of asteroids". Planetary and Space Science 73 (1): 98–118. doi:10.1016/j.pss.2012.03.009. Bibcode: 2012P&SS...73...98C. 
  11. ↑ 11.0 11.1 11.2 11.3 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)
  12. ↑ 12.0 12.1 12.2 12.3 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T. et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal 152 (3): 12. doi:10.3847/0004-6256/152/3/63. Bibcode: 2016AJ....152...63N. 
  13. ↑ 13.0 13.1 13.2 13.3 13.4 13.5 "LCDB Data for (1313) Berna". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1313%7CBerna. 
  14. ↑ 14.0 14.1 Behrend, R.; Roy, R.; Sposetti, S.; Waelchli, N.; Pray, D.; Berger, N. et al. (February 2004). "(1313) Berna". IAU Circ. 8292 (8292): 3. Bibcode: 2004IAUC.8292....3B. 
  15. ↑ 15.0 15.1 Behrend, R.; Bernasconi, L.; Roy, R.; Klotz, A.; Colas, F.; Antonini, P. et al. (February 2006). "Four new binary minor planets: (854) Frostia, (1089) Tama, (1313) Berna, (4492) Debussy". Astronomy and Astrophysics 446 (3): 1177–1184. doi:10.1051/0004-6361:20053709. Bibcode: 2006A&A...446.1177B. http://www.aanda.org/articles/aa/pdf/2006/06/aa3709-05.pdf. Retrieved 16 January 2017. 
  16. ↑ 16.0 16.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1313) Berna". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001313. 
  17. ↑ 17.0 17.1 17.2 17.3 17.4 Marchis, F.; Enriquez, J. E.; Emery, J. P.; Mueller, M.; Baek, M.; Pollock, J. et al. (November 2012). "Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations". Icarus 221 (2): 1130–1161. doi:10.1016/j.icarus.2012.09.013. Bibcode: 2012Icar..221.1130M. 
  18. ↑ Johnston, Robert. "(131) Berna". http://www.johnstonsarchive.net/astro/astmoons/am-01313.html. 
Cite error: <ref> tag with name "Johnston-Asteroids-with-Satellites" defined in <references> is not used in prior text.

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