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1421 Esperanto

From Wikipedia, the free encyclopedia
Dark background asteroid

1421 Esperanto
Discovery[1]
Discovered byY. Väisälä
Discovery siteTurku Obs.
Discovery date18 March 1936
Designations
(1421) Esperanto
Named after
Esperanto[1]
(artificial language)
1936 FQ · 1931 HC
1958 GD · A906 UD
A917 XD · A920 GD
main-belt[1][2] · (outer)
background[3][4]
Orbital characteristics[2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc111.92yr (40,879 d)
Aphelion3.3505AU
Perihelion2.8280 AU
3.0893 AU
Eccentricity0.0846
5.43 yr (1,983 d)
77.705°
0° 10m 53.4s / day
Inclination9.8030°
42.595°
163.18°
Physical characteristics
43.31±3.1 km[5]
51.95±10.21 km[6][7]
56.68±0.96 km[8]
62.06±17.35 km[9]
64.37±25.60 km[10]
21.982±0.005 h[11]
0.03[9][10]
0.042[8]
0.0714±0.011[5]
0.098[6][7]
C(assumed)[12]
9.56[7]
10.30[6][8][9]
10.4[1][2]
10.42[10]

1421 Esperanto, provisional designation1936 FQ, is a dark backgroundasteroid from the outer regions of theasteroid belt, approximately 55 kilometers (34 miles) in diameter. It was discovered on 18 March 1936, by Finnish astronomerYrjö Väisälä at theIso-Heikkilä Observatory in Turku, southwest Finland. The presumedC-type asteroid has arotation period of nearly 22 hours.[12] It was named for the artificial languageEsperanto.[1]

Orbit and classification

[edit]

Esperanto has been determined a non-family asteroid from the main belt'sbackground population by means of modernHCM-analysis, after it had previously been grouped to theEos family byZappalà in the 1990s.[3][4]

It orbits the Sun in theouter asteroid belt at a distance of 2.8–3.4 AU once every 5 years and 5 months (1,983 days;semi-major axis of 3.09 AU). Its orbit has aneccentricity of 0.08 and aninclination of 10° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1906 UD atHeidelberg Observatory in October 1906, almost 30 years prior to its official discovery observation at Turku.[1]

Naming

[edit]

Thisminor planet was named by the discoverer after theconstructed language,Esperanto, which was created by inventor and writer,Ludwik Lejzer Zamenhof (1859–1917), who used the pseudonym "Doktoro Esperanto".[1] The discoverer also named another asteroid,1462 Zamenhof, directly after the inventor. Both asteroids are considered to be the most remoteZamenhof-Esperanto objects. The officialnaming citation was published by theMinor Planet Center in January 1956 (M.P.C. 1350).[13]

Physical characteristics

[edit]

Esperanto is an assumed, carbonaceousC-type asteroid.[12]

Rotation period

[edit]

In March 2012, a rotationallightcurve ofEsperanto was obtained fromphotometric observations by Andrea Ferrero at the Bigmuskie Observatory (B88) in northern Italy. Lightcurve analysis gave arotation period of21.982±0.005 hours with a brightness amplitude of 0.15magnitude (U=3-).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Esperanto measures between 43.3 and 64.3 kilometers in diameter and its surface has analbedo between 0.03 and 0.098.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0714 and a diameter of 43.31 kilometers based on anabsolute magnitude of 10.3.[12][5]

References

[edit]
  1. ^abcdefg"1421 Esperanto (1936 FQ)".Minor Planet Center. Retrieved9 December 2018.
  2. ^abcd"JPL Small-Body Database Browser: 1421 Esperanto (1936 FQ)" (2018-09-18 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 August 2020. Retrieved9 December 2018.
  3. ^ab"Asteroid 1421 Esperanto".Small Bodies Data Ferret. Retrieved9 December 2018.
  4. ^ab"Asteroid (1421) Esperanto – Proper elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved4 December 2018.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved9 December 2018.
  6. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR-A-COMPIL-5-NEOWISEDIAM-V1.0.Bibcode:2016PDSS..247.....M. Retrieved9 December 2018.
  7. ^abcdMasiero, 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.S2CID 46350317.
  8. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,Usui Fumihiko (2013).Mid-Infrared Asteroid Survey with AKARI [「あかり」衛星による小惑星の中間赤外線サーベイ] (Thesis). Vol. Thesis or Dissertation. p. 153(p.1-178).)
  9. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381.
  10. ^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.
  11. ^abFerrero, Andrea (July 2012). "Lightcurve Photometry of Six Asteroids".The Minor Planet Bulletin.39 (3):138–139.Bibcode:2012MPBu...39..138F.ISSN 1052-8091.
  12. ^abcd"LCDB Data for (1421) Esperanto". Asteroid Lightcurve Database (LCDB). Retrieved9 December 2018.
  13. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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