Home  

Random  

Nearby  



Log in  



Settings  



Donate  



About Wikipedia  

Disclaimers  



Wikipedia





221 Eos





Article  

Talk  



Language  

Watch  

Edit  





Eos (minor planet designation: 221 Eos) is a large main-belt asteroid that was discovered by Austrian astronomer Johann Palisa on January 18, 1882, in Vienna. In 1884, it was named after Eos, the Greek goddess of the dawn, to honour the opening of a new observatory that was hoped to bring about a new dawn for Viennese astronomy.[5]

221 Eos
3D model based on lightcurve data
Discovery
Discovered byJohann Palisa
Discovery date18 January 1882
Designations

MPC designation

(221) Eos
Pronunciation/ˈɒs/[1]

Named after

Eos

Alternative designations

A882 BA

Minor planet category

Main belt (Eos)
AdjectivesEoan /ˈ.ən/[2]
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc130.21 yr (47561 d)
Aphelion3.3249 AU (497.40 Gm)
Perihelion2.69594 AU (403.307 Gm)

Semi-major axis

3.01044 AU (450.355 Gm)
Eccentricity0.10447

Orbital period (sidereal)

5.22 yr (1907.8 d)

Average orbital speed

17.16 km/s

Mean anomaly

66.5202°

Mean motion

0° 11m 19.284s / day
Inclination10.880°

Longitude of ascending node

141.845°

Argument of perihelion

193.56°
Physical characteristics
Dimensions103.87±3.6 km[3]
103.52 ± 5.60 km[4]
Mass(5.87 ± 0.34) × 1018kg[4]

Mean density

10.10 ± 1.74 g/cm3[4]

Synodic rotation period

10.443 h (0.4351 d)

Geometric albedo

0.1400±0.010

Spectral type

K

Absolute magnitude (H)

7.67

The asteroid is orbiting the Sun with a semimajor axisof3.01 AU, a period of 5.22 years, and an eccentricity of 0.1. The orbital plane is inclined by 10.9° to the plane of the ecliptic. It has a mean cross-section of 104 km,[3] and is spinning with a rotation period of 10.4 hours. Based upon its spectral characteristics, this object is classified as a K-type asteroid. The orbital properties show it to be a member of the extensive Eos asteroid family, which is named after it.[6] The spectral properties of the asteroid suggest it may have come from a partially differentiated parent body.[7]

References

edit
  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  • ^ "Eoan". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  • ^ a b c "221 Eos". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Archived from the original on 13 September 2020. Retrieved 12 May 2016.
  • ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009, S2CID 119226456. See Table 1.
  • ^ Schmadel, Lutz (2003), Dictionary of Minor Planet Names, Springer Science & Business Media, p. 35, ISBN 9783540002383.
  • ^ Veeder, G. J.; et al. (March 1995), "Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry", Icarus, 114 (1): 186–196, Bibcode:1995Icar..114..186V, CiteSeerX 10.1.1.31.2739, doi:10.1006/icar.1995.1053.
  • ^ Mothé-Diniz, T.; Carvano, J. M. (November 2005), "221 Eos: a remnant of a partially differentiated parent body?", Astronomy and Astrophysics, 442 (2): 727–729, Bibcode:2005A&A...442..727M, doi:10.1051/0004-6361:20053551.
  • edit


  • t
  • e

  • Retrieved from "https://en.wikipedia.org/w/index.php?title=221_Eos&oldid=1190801480"
     



    Last edited on 19 December 2023, at 23:10  





    Languages

     


    Asturianu
     / Bân-lâm-gú
    Boarisch
    Català
    Deutsch
    Ελληνικά
    Español
    Esperanto
    Euskara
    فارسی
    Français
    Հայերեն
    Italiano
    Latina
    Lëtzebuergesch
    Magyar
    Македонски
    مصرى

    Нохчийн
    Norsk bokmål
    Norsk nynorsk
    Occitan
    Plattdüütsch
    Polski
    Português
    Română
    Русский
    Slovenčina
    Slovenščina
    Српски / srpski
    Srpskohrvatski / српскохрватски
    Suomi
    Svenska
    Tagalog
    Татарча / tatarça

    Türkçe
    Українська
    Tiếng Vit
    Yorùbá

     

    Wikipedia


    This page was last edited on 19 December 2023, at 23:10 (UTC).

    Content is available under CC BY-SA 4.0 unless otherwise noted.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Terms of Use

    Desktop