14 Irene Explained

Minorplanet:yes
Background:
  1. D6D6D6
14 Irene
Symbol: (historical)
Discoverer:John Russell Hind
Discovered:May 19, 1851
Mpc Name:(14) Irene
Alt Names:A906 QC;
A913 EA;
1952 TM
Pronounced:[1]
Adjective:Irenean (< Irenæan)
Named After:Irēnē
Mp Category:Main belt
Orbit Ref:[2]
Epoch:July 14, 2004 (JD 2453200.5)
Eccentricity:0.168
Inclination:9.106°
Arg Peri:96.473°
Asc Node:86.493°
Mean Anomaly:326.489°
Mean Diameter:152 km (Dunham)
155 ± 6 km
Mass:[3]
Density:
2.614 ± 0.396/0.483 g/cm
Rotation:[4]
Spectral Type:S
Magnitude:8.85[5] to 12.30
Abs Magnitude:6.
Albedo:0.159
Angular Size: to 0.052"

14 Irene is a large main-belt asteroid, discovered by the English astronomer John Russell Hind on May 19, 1851. It is orbiting the Sun at a distance of with a period of 1518.1762NaN2 and an eccentricity of 0.168. The orbital plane is tilted at an angle of 9.1° to the plane of the ecliptic.[2]

14 Irene was named after Irēnē, a personification of peace in Greek mythology. She was one of the Horae, daughter of Zeus and Themis. The name was suggested by Sir John Herschel.[6] Hind wrote,

"You will readily discover that this name [...] has some relation to this event (the Great Industrial Exhibition) which is now filling our metropolis [London] with the talent of all civilised nations, with those of Peace, the productions of Art and Science, in which all mankind must feel an interest."The Great Exhibition of the Works of Industry of All Nations in the Crystal Palace of Hyde Park, London, ran from May 1 until October 18, 1851.

Hind suggested that the symbol for the asteroid should be "A dove carrying an olive-branch, with a star on its head",[7] but it was hardly drawn before the use of graphical symbols to represent asteroids was dropped entirely.[8] It is in the pipeline for Unicode 17.0 as U+1CEC7 .[9] [10]

Observations from 2007 indicate that the rotation pole of 14 Irene lies close to the plane of the ecliptic, indicating it has an obliquity close to 90°.[11] The fairly flat Irenian lightcurves indicate somewhat spherical proportions. This is a stony S-type asteroid with a mean diameter of around 152 km.[3] [2] It is spinning with a rotation period of 15 hours.[11]

There have been seven reported stellar occultation events by Irene. The best is a three chord event observed in 2013.[12]

See also

References

External links

Notes and References

  1. Noah Webster (1884) A Practical Dictionary of the English Language
  2. Web site: 2008-04-14 last obs . JPL Small-Body Database Browser: 14 Irene . 2008-11-27.
  3. James . Baer . Steven . Chesley . Robert . Matson . Astrometric masses of 26 asteroids and observations on asteroid porosity . The Astronomical Journal . 141 . 5 . 2011 . 10.1088/0004-6256/141/5/143 . 2011AJ....141..143B . free .
  4. Web site: Asteroid Lightcurve Parameters . https://archive.today/20060614093519/http://www.psi.edu/pds/archive/lc.html . dead . 2006-06-14 . 2008-11-03 . Planetary Science Institute .
  5. Web site: AstDys (14) Irene Ephemerides . Department of Mathematics, University of Pisa, Italy . 2010-06-26 .
  6. Book: Schmadel, Lutz D.. Dictionary of minor planet names. 1. 5th . 2003. Springer-Verlag. Berlin Heidelberg New York. 3-540-00238-3. 16.
  7. Hind . John Russell . 1852 . From a Letter of Mr. Hind to the Editor . Astronomical Journal . 2 . 22–23 . 10.1086/100162 . 1851AJ......2...22H . free .
  8. http://aa.usno.navy.mil/faq/docs/minorplanets.php When did the asteroids become minor planets?
  9. Web site: Unicode request for historical asteroid symbols . Bala . Gavin Jared . Miller . Kirk . 18 September 2023 . unicode.org . Unicode . 26 September 2023 .
  10. Web site: Proposed New Characters: The Pipeline . Unicode . unicode.org . The Unicode Consortium . 6 November 2023 .
  11. New Lightcurves of 8 Flora, 13 Egeria, 14 Irene, 25 Phocaea 40 Harmonia, 74 Galatea, and 122 Gerda . Pilcher . Frederick . Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers . 36 . 4 . 133–136 . October 2009 . 2009MPBu...36..133P .
  12. Web site: Asteroid Data Sets . sbn.psi.edu . 2018-05-19 .