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13474 Vʹyus

From Wikipedia, the free encyclopedia
Main-belt asteroid

13474 Vʹyus
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date29 August 1973
Designations
(13474) Vʹyus
Named after
Yurij Sergeevich Vasil'ev
(Rector ofSPbSTU)[2]
1973 QO1 · 1956 SA
1990 RT4
main-belt[1][3] · (middle)[4]
background[5][6]
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc61.56yr (22,485 d)
Aphelion3.3863AU
Perihelion1.8591 AU
2.6227 AU
Eccentricity0.2911
4.25 yr (1,551 d)
267.15°
0° 13m 55.2s / day
Inclination7.8141°
317.29°
36.160°
Physical characteristics
6.922±0.351 km[7][8]
7.876±0.701 km[5]
6.587±0.001 h[9]
0.113±0.022[5]
0.147±0.020[7][8]
S/C(assumed)[4]
13.5[8]
13.7[1][3]

13474 Vʹyus, provisional designation1973 QO1, is a backgroundasteroid from the centralasteroid belt, approximately 7 kilometers (4.3 miles) in diameter. It was discovered on 29 August 1973, by Soviet astronomerTamara Smirnova at theCrimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula.[1] The asteroid has arotation period of 6.6 hours and is likely elongated in shape.[4] It was named after Yurij Sergeevich Vasil'ev, rector of the formerSaint Petersburg State Technical University in Russia.[1]

Orbit and classification

[edit]

Vʹyus is a non-family asteroid from the main belt'sbackground population.[5][6] It orbits the Sun in thecentral asteroid belt at a distance of 1.9–3.4 AU once every 4 years and 3 months (1,551 days;semi-major axis of 2.62 AU). Its orbit has aneccentricity of 0.29 and aninclination of 8° with respect to theecliptic.[3]

The body'sobservation arc begins with its first identification as1956 SA atGoethe Link Observatory in September 1956, almost 17 years prior to its official discovery observation at Nauchnyj.[1]

Naming

[edit]

Thisminor planet was named after Yurij Sergeevich Vasil'ev (Yurij Vasilyev; born 1929), expert inhydropower engineering and rector of the Saint Petersburg State Technical University (SPbSTU), now known as thePeter the Great St. Petersburg Polytechnic University in Russia. The name is formed by putting the surname first and then concatenating the threeCyrillic letters that form his initials —Vasil'evYurijSergeevich, ВЮС.[2] The officialnaming citation was published by theMinor Planet Center on 27 April 2002 (M.P.C. 45338).[10]

Physical characteristics

[edit]

The asteroid'sspectral type is unknown. The Lightcurve Data Base assumes anS- orC-type to be equally likely, using an averaged value for its albedo(see below).[4][a]

Rotation period

[edit]

In September 2007, a rotationallightcurve ofVʹyus was obtained fromphotometric observations by Maurice Clark at the Montgomery College Observatory in Maryland, United States. Lightcurve analysis gave a well-definedrotation period of 6.587 hours with a brightness amplitude of 0.85magnitude (U=3).[9] A high brightness amplitude typically indicates that the body has an elongated rather than spherical shape.

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Vʹyus measures 6.922 and 7.876 kilometers in diameter and its surface has analbedo of 0.147 and 0.113, respectively.[7][8][5] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 – a compromise value between thestony (0.20) andcarbonaceous (0.057) asteroid's, both abundant in the main belt's central region – and calculates a diameter of 7.65 kilometers based on anabsolute magnitude of 13.7.[4]

Notes

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  1. ^Asteroid Lightcurve Data Base (LCDB) – 2. Taxonomic Class, orbital class, and albedo. The LCDB generically assumes anS/C-type with an albedo of 0.10 for non-family main belt asteroids with asemi-major axis between 2.6 and 2.7.

References

[edit]
  1. ^abcdef"13474 Vʹyus (1973 QO1)".Minor Planet Center. Retrieved16 January 2019.
  2. ^abSchmadel, Lutz D. (2007). "(13474) Vʹyus".Dictionary of Minor Planet Names – (13474) Vʹyus.Springer Berlin Heidelberg. p. 800.doi:10.1007/978-3-540-29925-7_8828.ISBN 978-3-540-00238-3.
  3. ^abcd"JPL Small-Body Database Browser: 13474 Vʹyus (1973 QO1)" (2018-04-20 last obs.).Jet Propulsion Laboratory. Retrieved16 January 2019.
  4. ^abcde"LCDB Data for (13474) Vʹyus". Asteroid Lightcurve Database (LCDB). Retrieved19 October 2017.
  5. ^abcde"Asteroid 13474 Vʹyus".Small Bodies Data Ferret. Retrieved16 January 2019.
  6. ^ab"Asteroid (13474) Vʹyus – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved16 January 2019.
  7. ^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. Retrieved19 October 2017.
  8. ^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.
  9. ^abClark, Maurice (October 2008)."Asteroid Lightcurve Observations".The Minor Planet Bulletin.35 (4):152–154.Bibcode:2008MPBu...35..152C.ISSN 1052-8091. Retrieved19 October 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved19 October 2017.

External links

[edit]
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Authority control databasesEdit this at Wikidata
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