Astronomy:1335 Demoulina
_Demoulina.png) Shape model of Demoulina from its lightcurve | |
| Discovery[1] | |
|---|---|
| Discovered by | K. Reinmuth |
| Discovery site | Heidelberg Obs. |
| Discovery date | 7 September 1934 |
| Designations | |
| (1335) Demoulina | |
| Named after | Prof. Demoulin[2] (Belgian astronomer) |
| 1934 RE · 1954 RA | |
| Minor planet category | main-belt · (inner) Flora[3] · background[4] |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 82.66 yr (30,191 days) |
| |{{{apsis}}}|helion}} | 2.5854 AU |
| |{{{apsis}}}|helion}} | 1.8955 AU |
| 2.2404 AU | |
| Eccentricity | 0.1540 |
| Orbital period | 3.35 yr (1,225 days) |
| Mean anomaly | 255.64° |
| Mean motion | 0° 17m 38.04s / day |
| Inclination | 2.5472° |
| Longitude of ascending node | 172.62° |
| 198.89° | |
| Physical characteristics | |
| Dimensions | 6.35±1.43 km[5] 7.47 km (calculated)[3] 7.484±0.130 km[6] 7.684±0.133 km[7] |
| Rotation period | 2.59±0.05 h (poor)[8] 74.86±0.10 h[9] |
| Geometric albedo | 0.2073±0.0275[7] 0.218±0.043[6] 0.24 (assumed)[3] 0.26±0.14[5] |
| S (assumed)[3] | |
| Absolute magnitude (H) | 12.8[3] · 12.9[1][7] · 13.06[5] · 13.89±0.74[10] |
1335 Demoulina, provisional designation 1934 RE, is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. Discovered by Karl Reinmuth at Heidelberg Observatory in 1934, the asteroid was named after Prof. Demoulin, a Belgian astronomer at Ghent University. It has a slower-than average spin rate of nearly 75 hours.
Discovery
Demoulina was discovered on 7 September 1934, by German astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany.[11] Six nights later, it was independently discovered by Belgian astronomer Eugène Delporte at Uccle Observatory on 13 September 1934.[2] The Minor Planet Center only recognizes the first discoverer.[11]
Orbit and classification
Demoulina is a member of the Flora family (402), a giant asteroid family and the largest family of stony asteroids in the asteroid belt.[3] However, it is a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements.[4]
It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.6 AU once every 3 years and 4 months (1,225 days; semi-major axis of 2.24 AU). Its orbit has an eccentricity of 0.15 and an inclination of 3° with respect to the ecliptic.[1] The body's observation arc begins with its official discovery observation at Heidelberg in 1934.[11]
Physical characteristics
Demoulina is an assumed S-type asteroid.[3]
Rotation period
In February 2006, a rotational lightcurve of Demoulina was obtained from photometric observations by American astronomers Lawrence Molnar and Melissa Haegert at the Calvin–Rehoboth Observatory in New Mexico. Lightcurve analysis gave a rotation period of 74.86 hours with a brightness amplitude of 0.78 magnitude ({{{1}}}).[9] While not being a slow rotator, Demoulina's period is significantly longer than that for most asteroids. Its high brightness amplitude also indicates that it has an irregular or elongated shape.
Other photometric lightcurves which are based on a single night of observation are rated poorly ({{{1}}}).[8]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Demoulina measures between 6.35 and 7.684 kilometers in diameter and its surface has an albedo between 0.2073 and 0.26.[5][6][7]
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the parent body of the Flora family, and calculates a diameter of 7.47 kilometers based on an absolute magnitude of 12.8.[3]
Naming
This minor planet was named after Prof. Demoulin, a Belgian astronomer at Ghent University. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 121).[2]
References
- ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 1335 Demoulina (1934 RE)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001335.
- ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2007). "(1335) Demoulina". Dictionary of Minor Planet Names – (1335) Demoulina. Springer Berlin Heidelberg. p. 109. doi:10.1007/978-3-540-29925-7_1336. ISBN 978-3-540-00238-3.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 "LCDB Data for (1335) Demoulina". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=1335%7CDemoulina.
- ↑ 4.0 4.1 "Asteroid 1335 Demoulina – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1335.
- ↑ 5.0 5.1 5.2 5.3 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.
- ↑ 6.0 6.1 6.2 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. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 29 November 2017.
- ↑ 7.0 7.1 7.2 7.3 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.
- ↑ 8.0 8.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1335) Demoulina". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#001335.
- ↑ 9.0 9.1 Molnar, Lawrence A.; Haegert, Melissa J. (December 2007). "Lightcurve Analysis of Five Main-belt Asteroids at the Calvin-Rehoboth Observatory". The Minor Planet Bulletin 34 (4): 126–128. ISSN 1052-8091. Bibcode: 2007MPBu...34..126M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2007MPBu...34..126M. Retrieved 29 November 2017.
- ↑ 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. doi:10.1016/j.icarus.2015.08.007. Bibcode: 2015Icar..261...34V. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V. Retrieved 29 November 2017.
- ↑ 11.0 11.1 11.2 "1335 Demoulina (1934 RE)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1335.
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
- 1335 Demoulina at AstDyS-2, Asteroids—Dynamic Site
- 1335 Demoulina at the JPL Small-Body Database
 |  |
