1029 La Plata

Shape model of La Plata from its lightcurve

Discovery[1]
Discovered by| J. F. Hartmann
Discovery site| La Plata Obs.
Discovery date| 28 April 1924
Designations

MPC designation

| (1029) La Plata
Named after| La Plata[2] (city in Argentina
and discovering observatory)

Alternative designations

| 1924 RK * 1938 DR2
1969 OU * A916 UL
A916 UR
Minor planet category| main-belt[1][3] * (outer)
Koronis[4][5]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc| 100.68 yr (36,772 d)
|{{{apsis}}}|helion}}| 2.9715 AU
|{{{apsis}}}|helion}}| 2.8083 AU

Semi-major axis

| 2.8899 AU
Eccentricity| 0.0282
Orbital period| 4.91 yr (1,794 d)
Mean anomaly| 87.729°
Mean motion| 0° 12m 2.16s / day
Inclination| 2.4254°
Longitude of ascending node| 29.903°

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

| 142.56°
Physical characteristics
Mean diameter| 16.46±1.07 km[6]
19.32±2.72 km[7]
20.71 km (derived)[4]
20.78±1.9 km[8]
Rotation period| 14 h[9]
14.174±0.003 h[10]
15.310±0.003 h[11]
15.37 h[12]
Geometric albedo| 0.1655 (derived)[4]
0.1819±0.039[8]
0.229±0.246[7]
0.310±0.045[6]

Spectral type

| Tholen = S[3][4] * S[13]
B–V = 0.787[3]
U–B = 0.390[3]
Absolute magnitude (H)| 10.79[7] * 10.88[3][6][8]
10.99[4][12]
11.01±0.01[11]
11.37±0.60[13]

1029 La Plata, provisional designation 1924 RK, is a stony Koronis asteroid from the outer regions of the asteroid belt, approximately 20 kilometers (12 miles) in diameter. It was discovered on 28 April 1924, by German astronomer Johannes Hartmann at the La Plata Astronomical Observatory in Argentina.[1] It was named after the city of La Plata, Argentina, where the discovering observatory is located. The possibly elongated S-type asteroid has a rotation period of 15.31 hours.[3]

## 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

La Plata is a member of the Koronis family (605),[4][5] a prominent asteroid family with nearly co-planar ecliptical orbits and one of the largest families in the main belt at all.[14] It orbits the Sun in the outer asteroid belt at a distance of 2.8–3.0 AU once every 4 years and 11 months (1,794 days; semi-major axis of 2.89 AU), which is near the 5:2 resonance with Jupiter (2.82 AU). Its orbit has an eccentricity of 0.03 and an inclination of 2° with respect to the ecliptic.[3]

The asteroid was first observed as A916 UL and A916 UR at the observatories at Simeiz and Algiers in October 1916, respectively. Its observation arc begins with the latter observation at Algiers on 31 October 1916, more than 7 years prior its official discovery observation at La Plata.[1]

## Physical characteristics

In the Tholen classification, La Plata is a common, stony S-type asteroid,[3][4] which agrees with the overall spectral type for Koronian asteroids.[14]: 23 The photometric survey conducted by Pan-STARRS also characterized it as an S-type.[13]

### Rotation period

In October 2004, a rotational lightcurve of La Plata was obtained from photometric observations during an extensive survey of Koronian asteroids at seven different observatories in the United States. Lightcurve analysis gave a well-defined rotation period of 15.310 hours with a brightness variation of 0.58 magnitude ({{{1}}}).[11] Previous measurements from 1975 and 1983 showed a period of 14 and 15.37 hours, respectively ({{{1}}}).[9][12] Also in October 2004, an alternative period of 14.174 hours was obtained by French amateur astronomer Laurent Bernasconi ({{{1}}}).[10] The consolidated brightness amplitude of 0.26 to 0.58 magnitude indicates that the body's shape is somewhat elongated.[4]

### Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, La Plata measures between 16.46 and 20.78 kilometers in diameter and its surface has an albedo between 0.1819 and 0.310.[6][7][8] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1655 and a diameter of 20.71 kilometers based on an absolute magnitude of 10.99.[4]

## Naming

This minor planet was named after the city of La Plata, Argentina, where the discovering La Plata Astronomical Observatory is located. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 98).[2]

## References

1. ↑ 1.0 1.1 1.2 1.3 "1029 La Plata (1924 RK)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=1029. Retrieved 19 March 2018.
2. ↑ 2.0 2.1 Schmadel, Lutz D. (2007). "(1029) la Plata". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 88. doi:10.1007/978-3-540-29925-7_1030. ISBN 978-3-540-00238-3.
3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 "JPL Small-Body Database Browser: 1029 La Plata (1924 RK)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001029. Retrieved 19 March 2018.
4. ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 4.8 Template:Cite LCDB
5. ↑ 5.0 5.1 "Asteroid 1029 La Plata – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1029+La+Plata. Retrieved 24 October 2019.
6. ↑ 6.0 6.1 6.2 6.3 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)
7. ↑ 7.0 7.1 7.2 7.3 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. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M. Retrieved 19 March 2018.
8. ↑ 8.0 8.1 8.2 8.3 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode: 2004PDSS...12.....T. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019.
9. ↑ 9.0 9.1 Lagerkvist, C.-I. (March 1978). "Photographic photometry of 110 main-belt asteroids". Astronomy and Astrophysics Supplement Series 31: 361–381. Bibcode: 1978A&AS...31..361L. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1978A&AS...31..361L. Retrieved 19 March 2018.
10. ↑ 10.0 10.1 Behrend, Raoul. "Asteroids and comets rotation curves – (1029) La Plata". Geneva Observatory. http://obswww.unige.ch/~behrend/page3cou.html#001029. Retrieved 19 March 2018.
11. ↑ 11.0 11.1 11.2 Slivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T. et al. (May 2008). "Rotation rates in the Koronis family, complete to H≈11.2". Icarus 195 (1): 226–276. doi:10.1016/j.icarus.2007.11.019. Bibcode: 2008Icar..195..226S. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008Icar..195..226S. Retrieved 19 March 2018.
12. ↑ 12.0 12.1 12.2 Binzel, R. P. (October 1987). "A photoelectric survey of 130 asteroids". Icarus 72 (1): 135–208. doi:10.1016/0019-1035(87)90125-4. ISSN 0019-1035. Bibcode: 1987Icar...72..135B. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1987Icar...72..135B. Retrieved 19 March 2018.
13. ↑ 13.0 13.1 13.2 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 19 March 2018.
14. ↑ 14.0 14.1 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 9780816532131. Bibcode: 2015aste.book..297N.

## External links

* Lightcurve Database Query (LCDB), at www.minorplanet.info
* Dictionary of Minor Planet Names, Google books
* Asteroids and comets rotation curves, CdR – Geneva Observatory, Raoul Behrend
* Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
* 1029 La Plata at AstDyS-2, Asteroids—Dynamic Site
* Ephemeris * Observation prediction * Orbital info * Proper elements * Observational info
* 1029 La Plata at the JPL Small-Body Database
* Close approach * Discovery * Ephemeris * Orbit diagram * Orbital elements * Physical parameters

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