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14 Irene

Main-belt asteroid

14 Irene

Main-belt asteroid

FieldValue
minorplanetyes
background#D6D6D6
image14 Irene.png
captionA three dimensional model of 14 Irene from light curve inversion on the top and images of the asteroid on the bottom.
name14 Irene
symbol[[File:Irene symbol (bold).svg24pxAstronomical symbol of 14 Ireneclass=skin-invert]] (historical)
discovererJohn Russell Hind
discovery_siteGeorge Bishop's Observatory
discovered20 May 1851
mpc_name(14) Irene
alt_namesA906 QC;
A913 EA;
1952 TM
pronounced
adjectiveIrenean (
named_afterIrēnē
mp_categoryMain belt
orbit_ref
epoch21 November 2025 (JD 2461000.5)
semimajor2.588 AU
perihelion2.167 AU
aphelion3.009 AU
eccentricity0.163
period4.163 yr (1520.59 d)
inclination9.130°
arg_peri98.265°
asc_node86.010°
mean_anomaly12.926°
jupiter_moid2.016 AU
tisserand3.385
dimensions(167 × 153 × 139) ± 16 km
mean_diameter152 km (Dunham)
155 ± 6 km
mass
density
2.614 ± 0.396/0.483 g/cm
rotation0.6275 days{{cite web
urlhttp://www.psi.edu/pds/archive/lc.html
archive-urlhttps://archive.today/20060614093519/http://www.psi.edu/pds/archive/lc.html
url-statusdeadarchive-date=2006-06-14
titleAsteroid Lightcurve Parameters
accessdate2008-11-03publisher=Planetary Science Institute }}
spectral_typeS
magnitude8.85{{cite web
titleAstDys (14) Irene Ephemerides
publisherDepartment of Mathematics, University of Pisa, Italy
urlhttps://newton.spacedys.com/astdys/index.php?pc=1.1.3.1&n=14&oc=500&y0=2088&m0=4&d0=1&h0=0&mi0=0&y1=2088&m1=4&d1=2&h1=0&mi1=0&ti=1.0&tiu=days
accessdate2010-06-26 }} to 12.30
abs_magnitude6.
albedo0.159
angular_sizeto 0.052"

A913 EA; 1952 TM 155 ± 6 km

2.614 ± 0.396/0.483 g/cm | archive-url=https://archive.today/20060614093519/http://www.psi.edu/pds/archive/lc.html | url-status=dead |archive-date=2006-06-14

14 Irene () is a large main-belt asteroid, discovered by the English astronomer John Russell Hind on 20 May 1851. It is orbiting the Sun at a distance of with a period of 1518.176 days and an eccentricity of 0.168. The orbital plane is tilted at an angle of 9.1° to the plane of the ecliptic.

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°. The fairly flat Irenian lightcurves indicate somewhat spherical proportions. This is a stony S-type asteroid with a mean diameter of around 152 km. It is spinning with a rotation period of 15 hours.

There have been seven reported stellar occultation events by Irene. The best is a three chord event observed in 2013.{{Cite web

History

John R. Hind discovered Irene on 20 May 1851.

Irene was discovered by English astronomer John R. Hind on the very early morning of 20 May 1851 from George Bishop's Observatory in London, England. At that time, he was observing near the star Lalande 29490, around the 16th hour of right ascension and 10–15°S of declination in the constellation of Scorpius. For several years prior, he had examined this region of the sky as a nearby star had been erroneously omitted from Wölfer's star charts. Near Lalande 29490, Xi Scorpii, and 50 Librae, he noticed a pale blue object of about the ninth magnitude that had not been recorded before. Since such an object was unlikely to have gone unnoticed in prior sweeps of the area, he quickly suspected its non-stellar nature. This was confirmed by follow-up observations throughout that morning, and Hind announced his discovery of a new planet through The London Times on 21 May 1851. Further announcements of the discovery were published by journals such as Astronomische Nachrichten on 2 June 1851 and The Astronomical Journal on 5 June 1851. Irene was the fourth asteroid discovered by Hind and the fourteenth discovered in history. Hind would go on to discover a further six asteroids.

Naming

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. 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 1 May until 18 October 1851.

Symbol

Hind suggested that the symbol for the asteroid should be "A dove carrying an olive-branch, with a star on its head", but it was hardly drawn before the use of graphical symbols to represent asteroids was dropped entirely. It was included in Unicode 17.0 as U+1CEC7 𜻇 ([[File:Irene symbol (fixed width).svg|12px|class=skin-invert]]).

Orbit

Irene orbits the Sun at an average distance, or semi-major axis, of 2.59 astronomical units (AU), placing it in the main asteroid belt. Along its 4.16 year long orbit, its distance from the Sun varies from 2.17 AU at perihelion to 3.01 AU at aphelion due to its orbital eccentricity of 0.16. Its orbit is inclined by 9° with respect to the ecliptic plane, and it does not belong to any known asteroid family, classifying it as a background asteroid.

Notes

References

|doi-access=free

|doi-access=free

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|url-status = live |archive-url = https://web.archive.org/web/20250327192326/https://www.lindahall.org/about/news/scientist-of-the-day/annibale-de-gasparis/ |archive-date = 27 March 2025}}

| access-date = September 9, 2025 | url-status = live

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. [http://aa.usno.navy.mil/faq/docs/minorplanets.php When did the asteroids become minor planets?] {{webarchive. link. (2007-09-21)
  3. Hind, John Russell. (1852). "From a Letter of Mr. Hind to the Editor". Astronomical Journal.
  4. Schmadel, Lutz D.. (2003). "Dictionary of minor planet names". [[Springer-Verlag]].
  5. (18 September 2023). "Unicode request for historical asteroid symbols". Unicode.
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