1313 Berna
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.[a]
| Discovery[1] | |
|---|---|
| Discovered by | S. Arend |
| Discovery site | Uccle Obs. |
| Discovery date | 24 August 1933 |
| Designations | |
| (1313) Berna | |
Named after | Bern[2] (capital of Switzerland) |
| 1933 QG · 1926 EA A911 OA | |
| main-belt[1][3] · (middle) background[4][5] | |
| Orbital characteristics[3] | |
| Epoch 27 April 2019 (JD 2458600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 84.74 yr (30,953 d) |
| Aphelion | 3.2074 AU |
| Perihelion | 2.1112 AU |
| 2.6593 AU | |
| Eccentricity | 0.2061 |
| 4.34 yr (1,584 d) | |
| 241.65° | |
| 0° 13m 38.28s / day | |
| Inclination | 12.545° |
| 298.14° | |
| 99.773° | |
| Known satellites | 1(see 2nd infobox)[a] |
| Physical characteristics | |
Mean diameter | 13.12±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 density | 1.21±0.14 cm3[10] |
| 25.46 h[13][14][15][16] | |
| 0.13[12] 0.169[11] 0.185[7][8][9] 0.212[17] 0.245[6] | |
| S (assumed)[13] | |
| 11.55[6] 11.6[1][3][13] 11.69±0.12[17] 11.75[12] 11.80[7][9][11] | |
Orbit and classification edit
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 edit
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 edit
| Discovery[a] | |
|---|---|
| Discovered by | R. Behrend, R. Roy S. Sposetti |
| Discovery date | 6 February 2004 |
| Light-curve | |
| Orbital characteristics | |
| 25 km | |
| 25.464±0.001 h[17][14] | |
| 30 mas (maximum) | |
| Satellite of | 1313 Berna |
| Physical characteristics | |
| Dimensions | 8.37 km[18] |
| Δ0.51 fainter than prim. | |
| 12.8–13.0 | |
Lightcurve edit
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 (U=3).[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 (U=n.a.).[17]: 40 Other light-curves were also obtained by several amateur astronomers giving a period of 6, 25.4 and 25.45 hours, respectively (U=1/2-/3-).[16]
Asteroid moon edit
In February 2004, a satellite orbiting the asteroid was discovered. The moon, designated S/2004 (1313) 1, measures about 11 kilometers in diameter and orbits Berna at a distance of 35 kilometer once every 25 hours and 28 minutes. Since the lightcurve is synchronized with the eclipse events, at least one body of the binary system rotates synchronously with the orbital motion. It was identified based on light-curve observations taken in February 2004 by several astronomers, including Raoul Behrend at Geneva Observatory, Stefano Sposetti, René Roy, Donald Pray, Christophe Demeautis, Daniel Matter, Alain Klotz and others.[a][14] Although the IAUC was released on 23 February 2004, the announcement was already made on 12 February 2004. There are several hundreds of asteroids known to have satellites (also see Category:Binary asteroids).[19]
Diameter and albedo edit
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 edit
- ^ a b c d 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 edit
- ^ a b c d e f "1313 Berna (1933 QG)". Minor Planet Center. Retrieved 11 December 2018.
- ^ a b c 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.
- ^ a b c d "JPL Small-Body Database Browser: 1313 Berna (1933 QG)" (2018-05-23 last obs.). Jet Propulsion Laboratory. Retrieved 11 December 2018.
- ^ a b "Asteroid 1313 Berna". Small Bodies Data Ferret. Retrieved 11 December 2018.
- ^ a b "Asteroid (1313) Berna – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 11 December 2018.
- ^ a b c d 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. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317.
- ^ a b c 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. Retrieved 11 December 2018.
- ^ a b c 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. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. S2CID 118745497.
- ^ a b c d 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. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 35447010. (catalog)
- ^ a b c Carry, B. (December 2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. Bibcode:2012P&SS...73...98C. doi:10.1016/j.pss.2012.03.009. S2CID 119226456.
- ^ a b c d 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. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
- ^ a b c d 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. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63.
- ^ a b c d e f "LCDB Data for (1313) Berna". Asteroid Lightcurve Database (LCDB). Retrieved 16 January 2017.
- ^ a b c 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.
- ^ a b 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" (PDF). Astronomy and Astrophysics. 446 (3): 1177–1184. Bibcode:2006A&A...446.1177B. doi:10.1051/0004-6361:20053709. Retrieved 16 January 2017.
- ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (1313) Berna". Geneva Observatory. Retrieved 16 January 2017.
- ^ a b c d e 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. arXiv:1604.05384. Bibcode:2012Icar..221.1130M. doi:10.1016/j.icarus.2012.09.013. S2CID 161887.
- ^ Johnston, Robert. "(131) Berna". johnstonsarchive.net. Retrieved 28 May 2015.
- ^ Wm. Robert Johnston (1 November 2015). "Asteroids with Satellites". Johnston's Archive. Retrieved 24 November 2015.
External links edit
- IAUC 8292
- Behrend 2005, Four new binary Minor Planets
- Asteroids with Satellites, Robert Johnston, johnstonsarchive.net
- Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)–(5000) – Minor Planet Center
- 1313 Berna at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
- 1313 Berna at the JPL Small-Body Database