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1569 Evita

From Wikipedia, the free encyclopedia
Dark background asteroid

1569 Evita
Discovery[1]
Discovered byM. Itzigsohn
Discovery siteLa Plata Obs.
Discovery date3 August 1948
Designations
(1569) Evita
Named after
Eva Perón
(First Lady of Argentina)[2]
1948 PA · 1936 KE
1947 LA · 1976 SJ10
main-belt · (outer)
background[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.65 yr (25,075 days)
Aphelion3.5669AU
Perihelion2.7267 AU
3.1468 AU
Eccentricity0.1335
5.58yr (2,039 days)
95.582°
0° 10m 35.76s / day
Inclination12.267°
99.509°
249.74°
Physical characteristics
Dimensions36.346±0.208 km[4]
0.047±0.007[5]
11.2[1]

1569 Evita (provisional designation1948 PA) is a dark backgroundasteroid from the outer regions of theasteroid belt, approximately 36 kilometers in diameter. It was discovered on 3 August 1948, by astronomerMiguel Itzigsohn at theLa Plata Astronomical Observatory in Argentina.[6] The asteroid was named afterEva Perón.[2]

Orbit and classification

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Based on thehierarchical clustering method, Evita is a non-family asteroid of the main belt'sbackground population.[3] It orbits the Sun in theouter main-belt at a distance of 2.7–3.6 AU once every 5 years and 7 months (2,039 days). Its orbit has aneccentricity of 0.13 and aninclination of 12° with respect to theecliptic.[1]

The asteroid was first identified as1936 KE at theJohannesburg Observatory in May 1936. The body'sobservation arc begins with its official discovery observation at La Plata.[6]

Physical characteristics

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Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Evita measures 36.346 kilometers in diameter and its surface has analbedo of 0.047.[4][5] An albedo near 0.05 is typical for carbonaceousC-type asteroids which dominate the outer asteroid belt. It has anabsolute magnitude of 11.2.[1]

Rotation period

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As of 2017, no rotationallightcurve of Evita has been obtained from photometric observations. The asteroid'srotation period andaxis, as well as its shape remain unknown.[7]

Naming

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Thisminor planet was named after the First Lady of Argentina,Eva Perón (1919–1952), who was commonly known by the affectionate Spanish diminutive form of her name, Evita. She was the wife of PresidentJuan Perón (1895–1974) of Argentina.[2]

The discoverer also named the asteroids1581 Abanderada,1582 Martir,1588 Descamisada and1589 Fanatica in tribute to Eva Perón.[2] The officialnaming citation was published by theMinor Planet Center in February 1951 (M.P.C. 519).[8]

References

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  1. ^abcde"JPL Small-Body Database Browser: 1569 Evita (1948 PA)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved12 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1569) Evita".Dictionary of Minor Planet Names – (1569) Evita.Springer Berlin Heidelberg. p. 124.doi:10.1007/978-3-540-29925-7_1570.ISBN 978-3-540-00238-3.
  3. ^ab"Asteroid 1569 Evita – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^abMasiero, 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. Retrieved12 September 2017.
  5. ^abMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved12 September 2017.
  6. ^ab"1569 Evita (1948 PA)".Minor Planet Center. Retrieved12 September 2017.
  7. ^"LCDB Data for (1569) Evita". Asteroid Lightcurve Database (LCDB). Retrieved12 September 2017.
  8. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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