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1199 Geldonia

1199 Geldonia, provisional designation 1931 RF, is an Eoan asteroid from the outer regions of the asteroid belt, approximately 32 kilometers in diameter. It was discovered on 14 September 1931, by Belgian astronomer Eugène Delporte at the Royal Observatory of Belgium in Uccle.[11] The asteroid was named after the Belgian town of Jodoigne.[2]

1199 Geldonia
Discovery[1]
Discovered byE. Delporte
Discovery siteUccle Obs.
Discovery date14 September 1931
Designations
(1199) Geldonia
Pronunciation/ɡɛlˈdniə/
Named after
Jodoigne[2]
(Belgian city)
1931 RF · 1930 MB
1946 OH · 1958 WC
A921 TF
main-belt · (outer)
Eos[3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc95.48 yr (34,873 days)
Aphelion3.1016 AU
Perihelion2.9337 AU
3.0177 AU
Eccentricity0.0278
5.24 yr (1,915 days)
324.45°
0° 11m 16.8s / day
Inclination8.7917°
235.63°
291.33°
Physical characteristics
Dimensions30.395±0.243 km[5]
31.25±3.0 km [3][6]
32.858±0.315 km[7]
35.88±0.50 km[8]
36.08±0.58 km[9]
28.3±0.2 h[10]
0.098±0.004[9]
0.098±0.010[8]
0.1182±0.0108[7]
0.1299±0.029[6][3]
Tholen = CGTP:[1][3]
B–V = 0.760[1]
U–B = 0.330[1]
10.36[1][3][6][7][8][9]

Orbit and classification edit

Geldonia is a member the Eos family (606),[4] the largest asteroid family of the outer main belt consisting of nearly 10,000 asteroids.[12]: 23  It orbits the Sun at a distance of 2.9–3.1 AU once every 5 years and 3 months (1,915 days). Its orbit has an eccentricity of 0.03 and an inclination of 9° with respect to the ecliptic.[1]

The body's observation arc begins with its first identification as A921 TF at Heidelberg Observatory in October 1921, almost 10 years prior to its official discovery observation at Uccle.[11]

Physical characteristics edit

In the Tholen classification, Geldonia has an ambiguous spectral type, closest to a carbonaceous C-type asteroid with some similarities to the G-, T- and the primitive P-type asteroids, and was flagged as a nosy spectrum (CGTP:).[1][3] The overall spectral type for members of the Eoan family on the other hand is that of a K-type.[12]: 23 

Rotation period edit

In November 2010, a rotational lightcurve of Geldonia was obtained from photometric observations by Italian astronomer Silvano Casulli. Lightcurve analysis gave a longer-than-average rotation period of 28.3 hours with a brightness amplitude of 0.11 magnitude (U=2-). While not being a slow rotator, which have periods longer than 100 hours, Geldonia's spin rate is still longer than that of most minor planets, which typically rotate between 2 and 20 hours once around their axis.

Diameter and albedo edit

According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Geldonia measures between 30.395 and 36.08 kilometers in diameter and its surface has an albedo between 0.098 and 0.1182.[5][7][8][9]

The Collaborative Asteroid Lightcurve Link adopts the results obtained by Infrared Astronomical Satellite, that is, an albedo of 0.1299 and a diameter of 31.25 kilometers based on an absolute magnitude of 10.36.[3][6]

Naming edit

This minor planet was named after the Belgian town of Jodoigne, also known by its Latin name of Geldenaken (hence the asteroid's name of "Geldonia"). It is the native town of the discoverer Eugène Delporte. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 111).[2]

References edit

  1. ^ a b c d e f g h "JPL Small-Body Database Browser: 1199 Geldonia (1931 RF)" (2017-03-29 last obs.). Jet Propulsion Laboratory. Retrieved 28 September 2017.
  2. ^ a b c Schmadel, Lutz D. (2007). "(1199) Geldonia". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 100. doi:10.1007/978-3-540-29925-7_1200. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f g "LCDB Data for (1199) Geldonia". Asteroid Lightcurve Database (LCDB). Retrieved 28 September 2017.
  4. ^ a b "Asteroid 1199 Geldonia – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
  5. ^ a b Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. Retrieved 28 September 2017.
  6. ^ a b c d 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. Retrieved 22 October 2019.
  7. ^ 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.
  8. ^ 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. Retrieved 28 September 2017.
  9. ^ 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)
  10. ^ Behrend, Raoul. "Asteroids and comets rotation curves – (1199) Geldonia". Geneva Observatory. Retrieved 28 September 2017.
  11. ^ a b "1199 Geldonia (1931 RF)". Minor Planet Center. Retrieved 28 September 2017.
  12. ^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.

External links edit

  • 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
  • 1199 Geldonia at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 1199 Geldonia at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

1199, geldonia, provisional, designation, 1931, eoan, asteroid, from, outer, regions, asteroid, belt, approximately, kilometers, diameter, discovered, september, 1931, belgian, astronomer, eugène, delporte, royal, observatory, belgium, uccle, asteroid, named, . 1199 Geldonia provisional designation 1931 RF is an Eoan asteroid from the outer regions of the asteroid belt approximately 32 kilometers in diameter It was discovered on 14 September 1931 by Belgian astronomer Eugene Delporte at the Royal Observatory of Belgium in Uccle 11 The asteroid was named after the Belgian town of Jodoigne 2 1199 GeldoniaDiscovery 1 Discovered byE DelporteDiscovery siteUccle Obs Discovery date14 September 1931DesignationsMPC designation 1199 GeldoniaPronunciation ɡ ɛ l ˈ d oʊ n i e Named afterJodoigne 2 Belgian city Alternative designations1931 RF 1930 MB1946 OH 1958 WCA921 TFMinor planet categorymain belt outer Eos 3 4 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc95 48 yr 34 873 days Aphelion3 1016 AUPerihelion2 9337 AUSemi major axis3 0177 AUEccentricity0 0278Orbital period sidereal 5 24 yr 1 915 days Mean anomaly324 45 Mean motion0 11m 16 8s dayInclination8 7917 Longitude of ascending node235 63 Argument of perihelion291 33 Physical characteristicsDimensions30 395 0 243 km 5 31 25 3 0 km 3 6 32 858 0 315 km 7 35 88 0 50 km 8 36 08 0 58 km 9 Synodic rotation period28 3 0 2 h 10 Geometric albedo0 098 0 004 9 0 098 0 010 8 0 1182 0 0108 7 0 1299 0 029 6 3 Spectral typeTholen CGTP 1 3 B V 0 760 1 U B 0 330 1 Absolute magnitude H 10 36 1 3 6 7 8 9 Contents 1 Orbit and classification 2 Physical characteristics 2 1 Rotation period 2 2 Diameter and albedo 3 Naming 4 References 5 External linksOrbit and classification editGeldonia is a member the Eos family 606 4 the largest asteroid family of the outer main belt consisting of nearly 10 000 asteroids 12 23 It orbits the Sun at a distance of 2 9 3 1 AU once every 5 years and 3 months 1 915 days Its orbit has an eccentricity of 0 03 and an inclination of 9 with respect to the ecliptic 1 The body s observation arc begins with its first identification as A921 TF at Heidelberg Observatory in October 1921 almost 10 years prior to its official discovery observation at Uccle 11 Physical characteristics editIn the Tholen classification Geldonia has an ambiguous spectral type closest to a carbonaceous C type asteroid with some similarities to the G T and the primitive P type asteroids and was flagged as a nosy spectrum CGTP 1 3 The overall spectral type for members of the Eoan family on the other hand is that of a K type 12 23 Rotation period edit In November 2010 a rotational lightcurve of Geldonia was obtained from photometric observations by Italian astronomer Silvano Casulli Lightcurve analysis gave a longer than average rotation period of 28 3 hours with a brightness amplitude of 0 11 magnitude U 2 While not being a slow rotator which have periods longer than 100 hours Geldonia s spin rate is still longer than that of most minor planets which typically rotate between 2 and 20 hours once around their axis Diameter and albedo edit According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA s Wide field Infrared Survey Explorer Geldonia measures between 30 395 and 36 08 kilometers in diameter and its surface has an albedo between 0 098 and 0 1182 5 7 8 9 The Collaborative Asteroid Lightcurve Link adopts the results obtained by Infrared Astronomical Satellite that is an albedo of 0 1299 and a diameter of 31 25 kilometers based on an absolute magnitude of 10 36 3 6 Naming editThis minor planet was named after the Belgian town of Jodoigne also known by its Latin name of Geldenaken hence the asteroid s name of Geldonia It is the native town of the discoverer Eugene Delporte The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 H 111 2 References edit a b c d e f g h JPL Small Body Database Browser 1199 Geldonia 1931 RF 2017 03 29 last obs Jet Propulsion Laboratory Retrieved 28 September 2017 a b c Schmadel Lutz D 2007 1199 Geldonia Dictionary of Minor Planet Names Springer Berlin Heidelberg p 100 doi 10 1007 978 3 540 29925 7 1200 ISBN 978 3 540 00238 3 a b c d e f g LCDB Data for 1199 Geldonia Asteroid Lightcurve Database LCDB Retrieved 28 September 2017 a b Asteroid 1199 Geldonia Nesvorny HCM Asteroid Families V3 0 Small Bodies Data Ferret Retrieved 26 October 2019 a b Masiero Joseph R Grav T Mainzer A K Nugent C R Bauer J M Stevenson R et al August 2014 Main belt Asteroids with WISE NEOWISE Near infrared Albedos The Astrophysical Journal 791 2 11 arXiv 1406 6645 Bibcode 2014ApJ 791 121M doi 10 1088 0004 637X 791 2 121 Retrieved 28 September 2017 a b c d 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 Retrieved 22 October 2019 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 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 Retrieved 28 September 2017 a b c d Usui Fumihiko Kuroda Daisuke Muller 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 Behrend Raoul Asteroids and comets rotation curves 1199 Geldonia Geneva Observatory Retrieved 28 September 2017 a b 1199 Geldonia 1931 RF Minor Planet Center Retrieved 28 September 2017 a b Nesvorny D Broz M Carruba V December 2014 Identification and Dynamical Properties of Asteroid Families Asteroids IV pp 297 321 arXiv 1502 01628 Bibcode 2015aste book 297N doi 10 2458 azu uapress 9780816532131 ch016 ISBN 9780816532131 External links editAsteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 1199 Geldonia at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 1199 Geldonia at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 1199 Geldonia amp oldid 1173731196, wikipedia, wiki, book, books, library,

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