17102 Begzhigitova

17102 BegzhigitovaDiscovery[1]

Discovered by| LINEAR
Discovery site| Lincoln Lab's ETS
Discovery date| 10 May 1999
Designations

MPC designation

| (17102) Begzhigitova
Named after| Akmaral Begzhigitova[2]
(2003 ISEF awardee)

Alternative designations

| 1999 JB41 * 1990 TD3
1995 DN3
Minor planet category| main-belt * (inner)
Flora[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc| 25.80 yr (9,425 days)
|{{{apsis}}}|helion}}| 2.5479 AU
|{{{apsis}}}|helion}}| 1.8993 AU

Semi-major axis

| 2.2236 AU
Eccentricity| 0.1459
Orbital period| 3.32 yr (1,211 days)
Mean anomaly| 32.465°
Mean motion| 0° 17m 49.92s / day
Inclination| 4.2249°
Longitude of ascending node| 152.89°

|{{{apsis}}}|helion}}

| 238.09°
Physical characteristics
Dimensions| 2.218±0.106 km[5][6]
2.97 km (calculated)[3]
Rotation period| 5.341±0.001 h[7]
Geometric albedo| 0.24 (assumed)[3]
0.393±0.076[5][6]

Spectral type

| S (assumed)[3]
Absolute magnitude (H)| 14.8[1][3] * 14.9[6] * 15.10±0.31[8]

17102 Begzhigitova (provisional designation 1999 JB41) is a stony Florian asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter. It was discovered on 10 May 1999, by astronomers of the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico, United States.[9] The asteroid was named after Akmaral Begzhigitova, an ISEF awardee of 2003.[2]

## Contents

* 1 Orbit and classification
* 2 Physical characteristics
* 2.1 Rotation period
* 2.2 Diameter and albedo
* 3 Naming
* 4 References
* 5 External links

## Orbit and classification

Begzhigitova is a member of the Flora family (402),[3][4] a giant asteroid family and the largest family of stony asteroids in the main belt.[10]: 23 It orbits the Sun in the inner asteroid belt at a distance of 1.9–2.5 AU once every 3 years and 4 months (1,211 days). Its orbit has an eccentricity of 0.15 and an inclination of 4° with respect to the ecliptic.[1]

The body's observation arc begins with its first identification as 1990 TD3 at Palomar Observatory in October 1990, almost 9 years prior to its official discovery observation at Socorro.[9]

## Physical characteristics

Begzhigitova is an assumed common S-type asteroid,[3] in agreement with the overall spectral type of the Flora family.[10]: 23

### Rotation period

In February 2008, a rotational lightcurve of Begzhigitova at an apparent magnitude of only 17 was obtained from photometric observations at Modra Observatory in the Czech Republic. Lightcurve analysis gave a rotation period of 5.341 hours with a brightness amplitude of 0.3 magnitude ({{{1}}}).[7] However a longer period can not be ruled out.[7]

### Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Begzhigitova measures 2.218 kilometers in diameter and its surface has an albedo of 0.393.[5][6]

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 2.97 kilometers based on an absolute magnitude of 14.8.[3]

## Naming

This minor planet was named after Akmaral Begzhigitova (born 1985), an Intel International Science and Engineering Fair (ISEF) awardee in 2003. The Ceres Connection program names minor planets in honor of students in fifth through twelfth grades and their teachers. She was awarded 4th place for her mathematics team project. At the time, Begzhigitova attended the Institute of Mathematics, Almaty, Kazakhstan.[2] The official naming citation was published by the Minor Planet Center on 14 June 2004 (M.P.C. 52172).[11]

## References

1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 17102 Begzhigitova (1999 JB41)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2017102.
2. ↑ 2.0 2.1 2.2 Schmadel, Lutz D. (2006). "(17102) Begzhigitova [2.22, 0.14, 4.2]". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 106. doi:10.1007/978-3-540-34361-5_1124. ISBN 978-3-540-34361-5.
3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 "LCDB Data for (17102) Begzhigitova". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=17102|Begzhigitova.
4. ↑ 4.0 4.1 "Asteroid 17102 Begzhigitova – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=17102+Begzhigitova#Asteroid 17102 BegzhigitovaEAR-A-VARGBDET-5-NESVORNYFAM-V3.0.
5. ↑ 5.0 5.1 5.2 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 27 October 2017.
6. ↑ 6.0 6.1 6.2 6.3 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.
7. ↑ 7.0 7.1 7.2 Galad, Adrian; Kornos, Leonard (October 2008). "A Collection of Lightcurves from Modra: 2007 December- 2008 June". The Minor Planet Bulletin 35 (4): 144–146. ISSN 1052-8091. Bibcode: 2008MPBu...35..144G. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35..144G. Retrieved 27 October 2017.
8. ↑ 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 27 October 2017.
9. ↑ 9.0 9.1 "17102 Begzhigitova (1999 JB41)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=17102.
10. ↑ 10.0 10.1 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 978-0-8165-3213-1. Bibcode: 2015aste.book..297N.
11. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.

## 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 (15001)-(20000) – Minor Planet Center
* 17102 Begzhigitova at AstDyS-2, Asteroids—Dynamic Site
* Ephemeris * Observation prediction * Orbital info * Proper elements * Observational info
* 17102 Begzhigitova at the JPL Small-Body Database
* Close approach * Discovery * Ephemeris * Orbit diagram * Orbital elements * Physical parameters

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