Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

7317 Cabot

From Wikipedia, the free encyclopedia
Main-belt asteroid

7317 Cabot
Discovery[1]
Discovered byG. Kulin
Discovery siteKonkoly
Discovery date12 March 1940
Designations
(7317) Cabot
Named after
John Cabot[1]
(Italian explorer)
1940 ED · 1983 JH
1987 OV1
main-belt[1][2] · (inner)
background[3] · Flora[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc34.79yr (12,706 d)
Aphelion2.6836AU
Perihelion1.9780 AU
2.3308 AU
Eccentricity0.1514
3.56 yr (1,300 d)
283.55°
0° 16m 37.2s / day
Inclination3.9844°
182.64°
54.312°
Physical characteristics
3.62 km(calculated)[4]
3.66±0.86 km[5]
5.363±0.257 km[6][7]
2.237±0.0003 h[8]
0.185±0.034[6][7]
0.24±0.12[5]
0.24(assumed)[4]
S(assumed)[4]
13.8[7]
13.922±0.003(R)[8]
14.0[2]
14.08±1.52[9]
14.33[5]
14.37[4]

7317 Cabot, provisional designation1940 ED, is a backgroundasteroid in aresonance with Jupiter, located the inner regions of theasteroid belt, approximately 3.6 kilometers (2.2 miles) in diameter. It was discovered on 12 March 1940, by Hungarian astronomerGyörgy Kulin at theKonkoly Observatory in Budapest.[1] The presumedS-type asteroid has arotation period of 2.2 hours.[4] It was named after Italian explorerJohn Cabot.[1]

Orbit and classification

[edit]

Cabot is located in a 10:3orbital resonance with Jupiter (10/3J),[10] a mean-motion resonance of moderate order and a location of orbital instability. Asteroids in these resonances are known for their chaotic orbits with a relatively shortLyapunov time.[11] It is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theFlora family (402), a giantasteroid family and the largest family of stony asteroids in the main-belt.[4]

It orbits the Sun in theinner asteroid belt at a distance of 2.0–2.7 AU once every 3 years and 7 months (1,300 days;semi-major axis of 2.33 AU). Its orbit has aneccentricity of 0.15 and aninclination of 4° with respect to theecliptic.[2] The body'sobservation arc begins with its observation as1983 JH atKlet Observatory in May 1983, or more than 43 years after to its official discovery observation at Konkoly.[1]

Physical characteristics

[edit]

Cabot is an assumed, stonyS-type asteroid.[4]

Rotation period

[edit]

In January 2011, a fragmentary rotationallightcurve ofCabot was obtained fromphotometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave a poorly definedrotation period of 2.237 hours with a brightness amplitude of 0.10magnitude (U=1).[8] As of 2018, no secure period has been published.[4]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Cabot measures 3.66 and 5.363 kilometers in diameter and its surface has analbedo of 0.185 and 0.24, respectively.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 3.62 kilometers based on anabsolute magnitude of 14.37.[4]

Naming

[edit]

Thisminor planet was named after Italian explorerJohn Cabot (Giovanni Caboto; c. 1450–1499), who discovered the coast ofNorth America in 1497, the first recorded landfall since the Norse voyages. The Venetian navigator sailed from Bristol under the commission ofHenry VII of England.[1] The official naming citation was published by theMinor Planet Center on 20 June 1997 (M.P.C. 30101).[12]

References

[edit]
  1. ^abcdefg"7317 Cabot (1940 ED)".Minor Planet Center. Retrieved23 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 7317 Cabot (1940 ED)" (2018-02-25 last obs.).Jet Propulsion Laboratory. Retrieved23 May 2018.
  3. ^ab"Asteroid 7317 Cabot".Small Bodies Data Ferret. Retrieved23 May 2018.
  4. ^abcdefghij"LCDB Data for (7317) Cabot". Asteroid Lightcurve Database (LCDB). Retrieved23 May 2018.
  5. ^abcdNugent, 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.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  6. ^abcMasiero, 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.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497.
  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. (catalog)
  8. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929.
  9. ^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.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339.
  10. ^"(7317) Cabot – Proper Elements".AstDyS-2, Asteroids—Dynamic Site. Retrieved23 May 2018.
  11. ^Nesvorný, D.; Morbidelli, A. (December 1998)."Three-Body Mean Motion Resonances and the Chaotic Structure of the Asteroid Belt".The Astronomical Journal.116 (6):3029–3037.Bibcode:1998AJ....116.3029N.doi:10.1086/300632.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved23 May 2018.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=7317_Cabot&oldid=1293967721"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp