14 Irene

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14 Irene
Discovery A
Discoverer John Russell Hind
Discovery date May 19, 1851
Alternate
designations
B
A906 QC;
A913 EA;
1952 TM
Category Main belt
Orbital elements C
Epoch July 14, 2004 (JD 2453200.5)
Eccentricity (e) 0.168
Semi-major axis (a) 386.730 Gm (2.585 AU)
Perihelion (q) 321.602 Gm (2.150 AU)
Aphelion (Q) 451.858 Gm (3.020 AU)
Orbital period (P) 1518.176 d (4.16 a)
Mean orbital speed 18.52 km/s
Inclination (i) 9.106°
Longitude of the
ascending node
(Ω)
86.493°
Argument of
perihelion
(ω)
96.473°
Mean anomaly (M) 326.489°
Physical characteristics D
Dimensions 181.8 km [1]
Mass 6.3×1018 kg
Density 2 ? g/cm³
Surface gravity 0.051 m/s²
Escape velocity 0.096 km/s
Rotation period 0.6275 d[2]
Spectral class S-type asteroid [1]
Absolute magnitude 6.30
Albedo (geometric) 0.160[1]
Mean surface
temperature
~170 K
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14 Irene (eye-ree'-nee (key)) is a very large Main belt asteroid.

It was discovered by J. R. Hind on May 19, 1851 and named after Eirene, a personification of peace in Greek mythology, 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 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",[3] but an actual drawing of the symbol was never made before the use of graphical symbols to represent asteroids was dropped entirely.[4]

The fairly flat Irenian lightcurves indicate somewhat spherical proportions. There have been four reported stellar occultation events by Irene.

[edit] Aspects

Stationary,
retrograde
Opposition Distance to
Earth (AU)
Maximum
brightness (mag)
Stationary,
prograde
Conjunction
to Sun
4 April 2005 17 May 2005 1.27771 9.0 3 July 2005 18 January 2006
17 July 2006 5 September 2006 1.98973 10.6 31 October 2006 10 April 2007
7 October 2007 26 November 2007 1.75378 10.0 17 January 2008 24 July 2008
11 March 2009 20 April 2009 1.19745 8.9 6 June 2009 2 January 2010
5 July 2010 22 August 2010 1.92476 10.4 16 October 2010 29 March 2011
22 September 2011 12 November 2011 1.86045 10.2 5 January 2012 1 July 2012
14 February 2013 21 March 2013 1.17939 8.9 7 May 2013 15 December 2013
21 June 2014 8 August 2014 1.83305 10.2 30 September 2014 17 March 2015
9 September 2015 29 October 2015 1.94395 10.4 24 December 2015 12 June 2016
16 January 2017 20 February 2017 1.22621 9.0 6 April 2017 24 November 2017
6 June 2018 24 July 2018 1.71769 10.0 12 September 2018 4 March 2019
27 August 2019 17 October 2019 2.00134 10.5 12 December 2019 26 May 2020
17 December 2020 25 January 2021 1.32394 9.1 11 March 2021 29 October 2020

[edit] Reference

  1. ^ a b c http://spiff.rit.edu/richmond/parallax/phot/LCSUMPUB.TXT
  2. ^ http://www.psi.edu/pds/archive/lc.html
  3. ^ Hind, John Russell (1852). "From a Letter of Mr. Hind to the Editor". Astron. J. 2: 22-23.
  4. ^ http://aa.usno.navy.mil/hilton/AsteroidHistory/minorplanets.html
  • Gould, B. A., New planet, Astronomical Journal, Vol. 2, iss. 27, p. 22, June 1851


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