1374 Isora
| Discovery [1] | |
|---|---|
| Discovered by | E. Delporte |
| Discovery site | Uccle Obs. |
| Discovery date | 21 October 1935 |
| Designations | |
| (1374) Isora | |
Named after | Constructed female name ("Rosi" spelled backwards)[2] |
| 1935 UA | |
| Mars-crosser [1][3][4] | |
| Orbital characteristics [1] | |
| Epoch 16 February 2017 (JD 2457800.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 81.05 yr (29,604 days) |
| Aphelion | 2.8775 AU |
| Perihelion | 1.6230 AU |
| 2.2502 AU | |
| Eccentricity | 0.2788 |
| 3.38 yr (1,233 days) | |
| 44.987° | |
| 0° 17m 31.2s / day | |
| Inclination | 5.2943° |
| 302.56° | |
| 60.988° | |
| Earth MOID | 0.6290 AU |
| Physical characteristics | |
| Dimensions | 5.48 km (derived)[4] |
| 8±2 h[5] 36.699±0.001 h[6] | |
| 0.20 (assumed)[4] | |
| SMASS = Sq [1] · S [4][7][8] | |
| 13.00[8] · 13.3[1] · 13.32±0.32[7] · 13.67±0.15[4][5] | |
1374 Isora, provisional designation 1935 UA, is a stony asteroid and eccentric Mars-crosser from the innermost regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 21 October 1935, by Belgian astronomer Eugène Delporte at Uccle Observatory in Belgium.[3]
Orbit and classification
In the SMASS taxonomy, Isora is classified as a Sq-type, an intermediary between the abundant S and rather rare Q-type asteroids. It orbits the Sun at a distance of 1.6–2.9 AU once every 3 years and 5 months (1,233 days). Its orbit has an eccentricity of 0.28 and an inclination of 5° with respect to the ecliptic.[1] Isora's observation arc begins with its official discovery observation at Uccle, as no precoveries were taken and no prior identifications were made.[3]
Physical characteristics
In January 2014, a rotational light-curve of Isora was obtained by American astronomer Robert D. Stephens at the Center for Solar System Studies (CS3) in California. Light-curve analysis gave a longer than average rotation period of 36.699 hours with a brightness variation of 0.12 magnitude (U=2+). However, a second period solution of 18.35 hours is also possible.[6] The result supersedes photometric observations taken by Wiesław Z. Wiśniewski in 1989, which rendered a fragmentary light-curve with a period of 8 hours (U=1).[5]
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 5.48 kilometers using an absolute magnitude of 13.67.[4]
Naming
Isora is the backwards spelled feminine name "Rosi" with an appended "a".[2] Naming was proposed by Gustav Stracke (1887–1943) – astronomer at the German Astronomisches Rechen-Institut, and after whom the minor planet 1019 Strackea is named – and first cited by Paul Herget in his The Names of the Minor Planets in 1955 (H 125).[2]
References
- ^ a b c d e f "JPL Small-Body Database Browser: 1374 Isora (1935 UA)" (2016-11-08 last obs.). Jet Propulsion Laboratory. Retrieved 11 January 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(1374) Isora". Dictionary of Minor Planet Names – (1374) Isora. Springer Berlin Heidelberg. p. 111. doi:10.1007/978-3-540-29925-7_1375. ISBN 978-3-540-00238-3.
- ^ a b c "1374 Isora (1935 UA)". Minor Planet Center. Retrieved 11 January 2017.
- ^ a b c d e f "LCDB Data for (1374) Isora". Asteroid Lightcurve Database (LCDB). Retrieved 11 January 2017.
- ^ a b c Wisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995). "Photoelectric Observations of 125 Asteroids". Abstracts of the Lunar and Planetary Science Conference. 26: 1511. Bibcode:1995LPI....26.1511W. Retrieved 11 January 2017.
- ^ a b Stephens, Robert D. (July 2014). "Asteroids Observed from CS3: 2014 January - March". The Minor Planet Bulletin. 41 (3): 171–175. Bibcode:2014MPBu...41..171S. ISSN 1052-8091. Retrieved 11 January 2017.
- ^ a b Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 11 January 2017.
- ^ a b Carry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016). "Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry". Icarus. 268: 340–354. arXiv:1601.02087. Bibcode:2016Icar..268..340C. doi:10.1016/j.icarus.2015.12.047. Retrieved 11 January 2017.
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- 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
- 1374 Isora at AstDyS-2, Asteroids—Dynamic Site
- 1374 Isora at the JPL Small-Body Database
