19367 Pink Floyd

Last updated

19367 Pink Floyd
Discovery [1]
Discovered by ODAS
Discovery site CERGA Obs.
Discovery date3 December 1997
Designations
(19367) Pink Floyd
Named after
Pink Floyd [2]
(English rock band)
1997 XW3 ·1985 UZ2
1999 JH126
main-belt  ·(inner)
Orbital characteristics [1]
background [3]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 62.66 yr (22,888 d)
Aphelion 2.8466 AU
Perihelion 2.0439 AU
2.4452 AU
Eccentricity 0.1641
3.82 yr (1,397 days)
114.74°
0° 15m 28.08s / day
Inclination 3.6853°
91.599°
305.17°
Physical characteristics
Dimensions6.652±0.172 km [4]
0.048±0.013 [4]
14.6 [1]

    19367 Pink Floyd (provisional designation 1997 XW3) is a dark background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 3 December 1997, by European astronomers of the ODAS survey at the CERGA Observatory near Caussols, France. [5] The asteroid was named after the English rock band Pink Floyd. [2]

    Contents

    Orbit and classification

    Pink Floyd is a non-family asteroid from the background population. [3] It orbits the Sun in the inner main-belt at a distance of 2.0–2.8  AU once every 3 years and 10 months (1,397 days). Its orbit has an eccentricity of 0.16 and an inclination of 4° with respect to the ecliptic. [1]

    The asteroid was first identified as 1985 UZ2 at the discovering Caussols Observatory in October 1985. Its observation arc begins 43 years prior to its official discovery observation, with a precovery taken by the Digitized Sky Survey at Palomar Observatory in July 1954. [5]

    Physical characteristics

    Diameter and albedo

    According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Pink Floyd measures 6.652 kilometers in diameter and its surface has a low albedo of 0.048. [4] An albedo near 0.05 is typical for carbonaceous C-type asteroids, which are the dominant type in the outer region of the main belt, but rather unusual in the inner parts. Pink Floyd has an absolute magnitude of 14.6. [1]

    Rotation period

    As of 2017, no rotational lightcurve of Pink Floyd has been obtained from photometric observations. The asteroid's rotation period, spin axis and shape remain unknown. [1] [6]

    Naming

    This minor planet was named after the English rock band Pink Floyd, which released several astronomically themed songs such as "Interstellar Overdrive" and "Astronomy Domine". The band's album The Dark Side of the Moon (1973) became one of the best-selling records of all time. [2]

    The official naming citation was published by the Minor Planet Center on 6 August 2003 ( M.P.C. 49281). [7]

    Related Research Articles

    <span class="mw-page-title-main">15017 Cuppy</span>

    15017 Cuppy, provisional designation 1998 SS25, is a Florian asteroid from the inner regions of the asteroid belt, approximately 2 kilometers in diameter. It was discovered on 22 September 1998, by the Lowell Observatory Near-Earth-Object Search (LONEOS) at its Anderson Mesa Station, Arizona, United States. The asteroid was named for American humorist Will Cuppy.

    25924 Douglasadams (provisional designation 2001 DA42) is a Nysian asteroid from the inner regions of the asteroid belt, approximately 2.4 kilometers in diameter. It was discovered on 19 February 2001, by astronomers of the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site in New Mexico, United States. The asteroid was named for novelist Douglas Adams.

    51824 Mikeanderson, provisional designation 2001 OE30, is an Eoan asteroid in the outer region of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 19 July 2001, by astronomers of the Near-Earth Asteroid Tracking program at Palomar Observatory in California, United States. The asteroid was named for American astronaut and mission payload commander Mike Anderson, who died in the Space Shuttle Columbia disaster.

    19738 Calinger (provisional designation 2000 AS97) is a background asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter.

    <span class="mw-page-title-main">9971 Ishihara</span> Asteroid

    9971 Ishihara is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at Kitami Observatory on 16 April 1993, and named after Takahiro Ishihara, president of the astronomical society at Hiroshima.

    78816 Caripito, provisional designation 2003 PZ9, is a background asteroid from the outer region of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. The asteroid was discovered on 4 August 2003, by American amateur astronomer and professor of geophysics, Joseph Dellinger at the Needville Observatory in Texas, United States. It was named for the town of Caripito in Venezuela.

    3917 Franz Schubert, provisional designation 1961 CX, is a bright background asteroid from the inner regions of the asteroid belt, approximately 5 kilometers in diameter. It was discovered on 15 February 1961, by astronomer Freimut Börngen at the Karl Schwarzschild Observatory in Tautenburg, Germany. The asteroid was named after Austrian composer Franz Schubert.

    14335 Alexosipov, provisional designation 1981 RR3, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered by Soviet–Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on 3 September 1981. The asteroid was named after astronomer Alexandr Osipov.

    58097 Alimov, provisional designation 1976 UQ1, is a background asteroid and relatively slow rotator from the central region of the asteroid belt, approximately 4 kilometers in diameter.

    6247 Amanogawa, provisional designation 1990 WY3, is a background asteroid from the inner regions of the asteroid belt, approximately 7 kilometers (4 miles) in diameter. It was discovered on 21 November 1990, by Japanese amateur astronomers Kin Endate and Kazuro Watanabe at the Kitami Observatory. The X-type asteroid has a rotation period of 12.38 hours. It was named after the Amanogawa River on the island of Hokkaido, Japan.

    2126 Gerasimovich, provisional designation 1970 QZ, is a stony background asteroid from the inner regions of the asteroid belt, approximately 8 kilometers in diameter. It was discovered on 30 August 1970, by Soviet astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named after Russian astronomer Boris Gerasimovich.

    15350 Naganuma, provisional designation 1994 VB2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 4.3 kilometers (2.7 miles) in diameter. It was discovered on 3 November 1994, by Japanese astronomers Yoshio Kushida and Osamu Muramatsu at the Yatsugatake South Base Observatory. The likely S-type asteroid has a rotation period of 2.5 hours. It was named for the town of Naganuma in northern Japan.

    5656 Oldfield, provisional designation A920 TA, is a background asteroid from the inner regions of the asteroid belt, approximately 7.7 kilometers in diameter. It was discovered on 8 October 1920, by astronomer Walter Baade at the Bergedorf Observatory in Hamburg, Germany. The asteroid was named for English musician Mike Oldfield.

    13260 Sabadell, prov. designation: 1998 QZ15, is a stony Eunomia asteroid from the central region of the asteroid belt. It was discovered by Catalan amateur astronomers Ferran Casarramona and Antoni Vidal at the Montjoia Observatory (953), Barcelona, on 23 August 1998. The likely elongated asteroid measures approximately 5.3 kilometers (3.3 miles) in diameter and has a rotation period of 5.3 hours. It was named after the astronomical society "Agrupació Astronòmica de Sabadell".

    84882 Table Mountain (provisional designation 2003 CN16) is a bright background asteroid from the central region of the asteroid belt, approximately 3 kilometers (1.9 miles) in diameter. It was discovered on 1 February 2003, by American astronomer James Whitney Young at the Table Mountain Observatory near Wrightwood, California. The S/Q-type asteroid was later named after the discovering observatory.

    7776 Takeishi, provisional designation 1993 BF, is a background asteroid from the inner regions of the asteroid belt, approximately 6 kilometers in diameter. It was discovered on 20 January 1993, by Japanese astronomer Takeshi Urata at the Nihondaira Observatory in Japan. The assumed S-type asteroid has a rotation period of 8.9 hours. It was named after Japanese amateur astronomer Masanori Takeishi.

    <span class="mw-page-title-main">45300 Thewrewk</span>

    45300 Thewrewk (provisional designation 2000 AF45) is a dark background asteroid from the outer regions of the asteroid belt, approximately 13 kilometers in diameter. It was discovered on 1 January 2000, by astronomers Krisztián Sárneczky and László Kiss at the Piszkéstető Station of the Konkoly Observatory in Hungary. The asteroid was named after Hungarian astronomer Aurél Ponori Thewrewk.

    17035 Velichko (provisional designation 1999 FC10) is a Vestian asteroid from the inner regions of the asteroid belt, approximately 4.5 kilometers in diameter.

    37432 Piszkéstető (provisional designation 2002 AE11) is an Erigonian asteroid from the inner regions of the asteroid belt, approximately 4.6 kilometers (2.9 miles) in diameter. It was discovered on 11 January 2002, by the Hungarian astronomers Krisztián Sárneczky and Zsuzsanna Heiner at the Konkoly Observatory's Piszkéstető Station northeast of Budapest, Hungary. The asteroid was later named for the discovering observatory.

    10140 Villon, provisional designation 1993 SX4, is a Nysian asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3 miles) in diameter. It was discovered on 19 September 1993, by Belgian astronomer Eric Elst at the CERGA Observatory at Caussols in France. It was named after 15th-century French poet François Villon.

    References

    1. 1 2 3 4 5 6 "JPL Small-Body Database Browser: 19367 Pink Floyd (1997 XW3)" (2017-03-30 last obs.). Jet Propulsion Laboratory . Retrieved 13 September 2017.
    2. 1 2 3 Schmadel, Lutz D. (2006). "(19367) Pink Floyd [2.44, 0.16, 3.7]". Dictionary of Minor Planet Names – (19367) Pink Floyd, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 134. doi:10.1007/978-3-540-34361-5_1491. ISBN   978-3-540-34361-5.
    3. 1 2 "Asteroid 19367 Pink Floyd – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved 29 October 2019.
    4. 1 2 3 Masiero, 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 . Retrieved 13 September 2017.
    5. 1 2 "19367 Pink Floyd (1997 XW3)". Minor Planet Center. Retrieved 13 September 2017.
    6. "LCDB Data for (19367) Pink Floyd". Asteroid Lightcurve Database (LCDB). Retrieved 13 September 2017.
    7. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 13 September 2017.