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9344 Klopstock

From Wikipedia, the free encyclopedia
Asteroid

9344 Klopstock
Discovery[1]
Discovered byF. Börngen
L. D. Schmadel
Discovery siteKarl Schwarzschild Obs.
Discovery date12 September 1991
Designations
(9344) Klopstock
Named after
Friedrich Gottlieb Klopstock[1](German poet)
1991 RB4 · 1995 WK2
main-belt[1][2] · (inner)
background[3] · Vestian[4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc26.35yr (9,626 d)
Aphelion2.5711AU
Perihelion2.1575 AU
2.3643 AU
Eccentricity0.0875
3.64 yr (1,328 d)
342.64°
0° 16m 15.96s / day
Inclination5.0293°
340.39°
156.40°
Physical characteristics
3.66 km(calculated)[4]
17.05±1.5 km[5]
5.842±0.0031 h[6]
0.0116±0.002[5]
0.20(assumed)[4]
S(assumed)[4]
14.095±0.003(R)[6]
14.2[2]
14.55[4]
14.86±0.14[7]

9344 Klopstock, provisional designation1991 RB4, is a backgroundasteroid from the inner regions of theasteroid belt. It was discovered on 12 September 1991, by German astronomersFreimut Börngen andLutz Schmadel at theKarl Schwarzschild Observatory in Tautenburg, Germany. Poor observational data suggests that the asteroid is one of the darkest known objects with a diameter of approximately 17 kilometers (11 miles), while it is also an assumedstony asteroid with a much smaller diameter. It has arotation period of 5.84 hours and was named after German poetFriedrich Gottlieb Klopstock.[1][2][4]

Orbit and classification

[edit]

Klopstock is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] Based on osculating Keplerianorbital elements, the asteroid has also been classified as a member of theVesta family (401), one of the largestasteroid families of bright asteroids in the main-belt.[4]

It orbits the Sun in theinner main-belt at a distance of 2.2–2.6 AU once every 3 years and 8 months (1,328 days;semi-major axis of 2.36 AU). Its orbit has aneccentricity of 0.09 and aninclination of 5° with respect to theecliptic.[2] The body'sobservation arc begins with its official discovery observation at Tautenburg in September 1991.[1]

Physical characteristics

[edit]

Klopstock is an assumed, stonyS-type asteroid,[4] aspectral type contrary to the outstandingly low IRAS albedo(see below).

Rotation period

[edit]

In September 2013, a rotationallightcurve ofKlopstock was obtained fromphotometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 5.842 hours with a brightness amplitude of 0.38magnitude (U=2).[6]

Diameter and albedo

[edit]

According to the survey carried out by theInfrared Astronomical Satellite (IRAS) in the 1980s,Klopstock measures 17.05 kilometers in diameter and its surface has an exceptionally lowalbedo of 0.0116.[5] This would make it one of the darkest asteroid known to exist.[8] However, the result is derived from two IRAS-observations only.[5] TheCollaborative Asteroid Lightcurve Link disregards the IRAS-data and assumes a standard albedo for a stony asteroid of 0.20 and consequently calculates a smaller diameter of 3.66 kilometers based on anabsolute magnitude of 14.55.[4]

Naming

[edit]

Thisminor planet was named after German poetFriedrich Gottlieb Klopstock (1724–1803), an important figure in the literary style calledEmpfindsamkeit.[1] The official naming citation was published by theMinor Planet Center on 2 February 1999 (M.P.C. 33795).[9]

References

[edit]
  1. ^abcdef"9344 Klopstock (1991 RB4)".Minor Planet Center. Retrieved29 April 2018.
  2. ^abcde"JPL Small-Body Database Browser: 9344 Klopstock (1991 RB4)" (2018-01-19 last obs.).Jet Propulsion Laboratory. Retrieved29 April 2018.
  3. ^ab"Asteroid 9344 Klopstock – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  4. ^abcdefghi"LCDB Data for (9344) Klopstock". Asteroid Lightcurve Database (LCDB). Retrieved29 April 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.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  6. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015). "Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.
  7. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.
  8. ^"JPL Small-Body Database Search Engine: albedo < 0.02". JPL Solar System Dynamics. Retrieved29 April 2018.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 April 2018.

External links

[edit]
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