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3754 Kathleen

From Wikipedia, the free encyclopedia
Large background asteroid

3754 Kathleen
Discovery[1]
Discovered byC. W. Tombaugh
Discovery siteLowell Obs.
Discovery date16 March 1931
Designations
(3754) Kathleen
Named after
Kathleen Clifford[1]
(Discoverer's granddaughter)
1931 FM · 1925 BF
1929 WA1 · 1955 MR
1957 WH1 · 1959 CH1
1959 EC1 · 1963 WD
1977 KR · 1978 NM2
1982 DQ4 · 1985 UD4
1987 BK · A909 HE
main-belt[1][2] · (outer)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc108.53yr (39,639 d)
Aphelion3.4993AU
Perihelion2.8168 AU
3.1581 AU
Eccentricity0.1081
5.61 yr (2,050 d)
157.55°
0° 10m 32.16s / day
Inclination8.4535°
110.50°
55.593°
Physical characteristics
53.03 km(derived)[4]
53.23±1.8 km[5]
53.699±0.248 km[6]
54.283±1.200 km[7]
57.27±0.69 km[8]
58.64±20.04 km[9]
59.367±14.24 km[10]
11.16±0.01 h[11]
11.17±0.02 h[11]
11.18±0.01 h[12]
11.2±0.1 h[13]
0.0379±0.0217[10]
0.04±0.01[9]
0.0435(derived)[4]
0.054±0.002[8]
0.0599±0.0072[7]
0.061±0.006[6]
0.0624±0.005[5]
C(assumed)[4]
10.00[5][7][8]
10.30[9]
10.40[2][4][10]

3754 Kathleen, provisional designation1931 FM, is a large backgroundasteroid from the outer regions of theasteroid belt, approximately 55 kilometers (34 miles) in diameter. It was discovered at theLowell Observatory near Flagstaff, Arizona, on 16 March 1931, by American astronomerClyde Tombaugh, who named it after his granddaughterKathleen Clifford.[1] The assumedC-type asteroid has arotation period of 11.18 hours.[4] It is the second-highest numbered main-belt asteroid larger than 50 kilometers.[14]

Orbit and classification

[edit]

Kathleen is a non-family asteroid from the main belt'sbackground population.[3] It orbits the Sun in theouter main-belt at a distance of 2.8–3.5 AU once every 5 years and 7 months (2,050 days;semi-major axis of 3.16 AU). Its orbit has aneccentricity of 0.11 and aninclination of 8° with respect to theecliptic.[2] The body'sobservation arc begins with its first observations asA909 HE atHeidelberg Observatory in April 1909, nearly 22 years prior to its official discovery observation at Flagstaff.[1]

Physical characteristics

[edit]

Kathleen is an assumed carbonaceousC-type asteroid.[4]

Rotation period

[edit]

Several rotationallightcurves ofKathleen have been obtained fromphotometric observations since March 2004.[11][12][13] Analysis of the best-rated lightcurve gave arotation period of 11.18 hours with a consolidated brightness amplitude between 0.13 and 0.20magnitude (U=3-).[4][12]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Kathleen measures between 53.23 and 59.367 kilometers in diameter and its surface has analbedo between 0.0379 and 0.0624.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0435 and a diameter of 53.03 kilometers based on anabsolute magnitude of 10.4.[4] Besides3925 Tretʹyakov, it is the highest numbered main-belt asteroid larger than 50 kilometers in diameter, of which there are 642 bodies in total, according to theJPL SBDB.[14]

Naming

[edit]

Thisminor planet was named afterKathleen Willoughby Clifford, granddaughter of the discovererClyde Tombaugh (1906–1997).[1] The official naming citation was published by theMinor Planet Center on 28 May 1991 (M.P.C. 18306).[15]

References

[edit]
  1. ^abcdef"3754 Kathleen (1931 FM)".Minor Planet Center. Retrieved1 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 3754 Kathleen (1931 FM)" (2017-10-29 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 15 September 2020. Retrieved1 May 2018.
  3. ^ab"Asteroid 3754 Kathleen – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^abcdefgh"LCDB Data for (3754) Kathleen". Asteroid Lightcurve Database (LCDB). Retrieved1 May 2018.
  5. ^abcdTedesco, 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. Retrieved22 October 2019.
  6. ^abcMasiero, 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.S2CID 119293330.
  7. ^abcdMainzer, 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.S2CID 35447010.
  8. ^abcdUsui, 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)
  9. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381.
  10. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.S2CID 250780308.
  11. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (3754) Kathleen". Geneva Observatory. Retrieved1 May 2018.
  12. ^abcMansego, Enrique Arce; Rodriguez, Pedro Brines; de Haro, Juan Lozano; Chiner, Onofre Rodrigo; Silva, Alvaro Fornas; Porta, David Herrero; et al. (October 2016)."Eighteen Asteroids Lightcurves at Asteroides Observers (OBAS) – MPPD: 2016 March–May".The Minor Planet Bulletin.43 (4):332–336.Bibcode:2016MPBu...43..332M.ISSN 1052-8091. Retrieved1 May 2018.
  13. ^abTorno, Steven; Oliver, Robert Lemke; Ditteon, Richard (June 2008)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory – October 2007".The Minor Planet Bulletin.35 (2):54–55.Bibcode:2008MPBu...35...54T.ISSN 1052-8091. Retrieved1 May 2018.
  14. ^ab"JPL Small-Body Database Browser: diameter > 50 (km) and a < 4.6 (au)". Jet Propulsion Laboratory. Retrieved1 May 2018.
  15. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 May 2018.

External links

[edit]
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Authority control databasesEdit this at Wikidata
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