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5148 Giordano

From Wikipedia, the free encyclopedia
Main-belt asteroid

5148 Giordano
Discovery[1]
Discovered byC. J. van Houten
I. van Houten G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date17 October 1960
Designations
(5148) Giordano
Named after
Giordano Bruno[2][3]
(Italian friar and heretic)
5557 P-L · 1974 CS
1980 GC1
main-belt[1] · (outer)
background[4] · Themis[3]
Orbital characteristics[5]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc57.33yr (20,940 d)
Aphelion3.5690AU
Perihelion2.6606 AU
3.1148 AU
Eccentricity0.1458
5.50 yr (2,008 d)
301.66°
0° 10m 45.48s / day
Inclination1.1261°
346.73°
227.45°
Physical characteristics
6.06 km(calculated)[3]
8.112±0.388 km[6][7]
8.5±1.7 km[8]
7.824±0.0038 h[9]
0.07±0.03[8]
0.08(assumed)[3]
0.0889±0.0250[7]
0.089±0.025[6]
C[3]
13.7[7] · 13.90[5][8]
13.996±0.011(R)[9]
14.45[3]

5148 Giordano, provisional designation5557 P-L, is a backgroundasteroid from the outer regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 17 October 1960, by Dutch astronomer coupleIngrid andCornelis van Houten on photographic plates taken by Dutch–American astronomerTom Gehrels at thePalomar Observatory in California, United States.[1] It was named for Italian friar and hereticGiordano Bruno, who was burned at the stake in Rome in 1600.[2] The presumably carbonaceous Themistian asteroid has arotation period of 7.8 hours and possibly an elongated shape.[3]

Orbit and classification

[edit]

Giordano is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[4] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a Themistian asteroid that belongs to theThemis family (602), a very largefamily ofcarbonaceous asteroids, named after24 Themis.[3]

It orbits the Sun in theouter asteroid belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,008 days;semi-major axis of 3.11 AU). Its orbit has aneccentricity of 0.15 and aninclination of 1° with respect to theecliptic.[5] The body'sobservation arc begins at Palomar on 24 September 1960, less than a month prior to its official discovery observation.[1]

Physical characteristics

[edit]

Giordano is an assumed carbonaceousC-type asteroid derived from the overallspectral type for Themistian asteroids.[3]

Rotation period

[edit]

In September 2010, a rotationallightcurve of Giordano was obtained fromphotometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 7.824 hours with a brightness amplitude of 0.60magnitude, indicative for an elongated shape (U=2).[9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Giordano measures 8.112 and 8.5 kilometers in diameter and its surface has analbedo of 0.089 and 0.07, respectively.[6][7][8] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 6.06 kilometers based on anabsolute magnitude of 14.45.[3]

Palomar–Leiden survey

[edit]

Thesurvey designation "P-L" stands forPalomar–Leiden, named after Palomar Observatory andLeiden Observatory, which collaborated on the fruitfulPalomar–Leiden survey in the 1960s. Gehrels used Palomar'sSamuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped thephotographic plates to Ingrid and Cornelis van Houten at Leiden Observatory whereastrometry was carried out. The trio are credited with the discovery ofseveral thousand asteroid discoveries.[10]

Naming

[edit]

Thisminor planet was named after an Italian Dominican friarGiordano Bruno (1548–1600), a philosopher, mathematician, poet, and cosmological theorist who spent many years in London, where several of his papers were published.[2]

Bruno was convinced that theCopernican heliocentric rather than theGeocentric model was correct, and proposed that other worlds, on which people could live, might exist around other stars. This brought him in conflict with the church. He was found guilty of heresy by the Roman Inquisition and was burned at the stake in Rome in 1600. The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22507). The asteroid's number, 5148, is a permutation of his birth year (1548). The lunar craterGiordano Bruno was also named in his honor.[2][11] Another asteroid,13223 Cenaceneri, was named after Bruno's work "The Dinner of the Ashes" (Italian:La Cena delle Ceneri), where he discusses the possibility of an infinite number of worlds in the universe.

References

[edit]
  1. ^abcd"5148 Giordano (5557 P-L)".Minor Planet Center. Retrieved26 March 2018.
  2. ^abcdSchmadel, Lutz D. (2007). "(5148) Giordano".Dictionary of Minor Planet Names – (5148) Giordano. Springer Berlin Heidelberg. p. 443.doi:10.1007/978-3-540-29925-7_5000.ISBN 978-3-540-00238-3.
  3. ^abcdefghij"LCDB Data for (5148) Giordano". Asteroid Lightcurve Database (LCDB). Retrieved26 March 2018.
  4. ^ab"Asteroid 5148 Giordano – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^abc"JPL Small-Body Database Browser: 5148 Giordano (5557 P-L)" (2018-01-23 last obs.).Jet Propulsion Laboratory. Retrieved26 March 2018.
  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. Retrieved26 March 2018.
  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.
  8. ^abcdAlí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016)."Differences between the Pallas collisional family and similarly sized B-type asteroids".Astronomy and Astrophysics.591: 11.Bibcode:2016A&A...591A..14A.doi:10.1051/0004-6361/201527660.hdl:11336/63614. Retrieved26 March 2018.
  9. ^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. Retrieved26 March 2018.
  10. ^"Minor Planet Discoverers".Minor Planet Center. 2018. Retrieved26 March 2018.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 March 2018.

External links

[edit]
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