To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

1383 Limburgia

From Wikipedia, the free encyclopedia

1383 Limburgia
Discovery[1]
Discovered byH. van Gent
Discovery siteJohannesburg Obs.
(Leiden Southern Station)
Discovery date9 September 1934
Designations
(1383) Limburgia
Named after
Limburg (Dutch province)[2]
1934 RV · 1929 UQ
1929 VJ · A923 PA
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc93.24 yr (34,057 days)
Aphelion3.6641 AU
Perihelion2.4903 AU
3.0772 AU
Eccentricity0.1907
5.40 yr (1,972 days)
81.370°
0° 10m 57.36s / day
Inclination0.0526°
194.03°
164.68°
Physical characteristics
Dimensions22.18 km (derived)[3]
22.84±6.23 km[4]
23.399±0.039 km[5]
24.29±0.16 km[6]
25.186±0.086 km[7]
26.66±0.27 km[8]
5 h[9]
0.039±0.010[8]
0.04±0.00[6]
0.0419±0.0053[7]
0.05±0.05[4]
0.0569 (derived)[3]
0.076±0.007[5]
C[3]
11.5[7] · 12.0[1][3][4][8] · 12.20±0.21[10] · 12.23[6]

1383 Limburgia, provisional designation 1934 RV, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 23 kilometers in diameter. It was discovered on 9 September 1934, by Dutch astronomer Hendrik van Gent at the Leiden Southern Station, annex to the Johannesburg Observatory in South Africa.[11] It is named for the Dutch province Limburg.[2]

Classification and orbit

Limburgia is a dark C-type asteroid. It orbits the Sun at a distance of 2.5–3.7 AU once every 5 years and 5 months (1,972 days). Its orbit has an eccentricity of 0.19 and an inclination of 0° with respect to the ecliptic, which means that it is coplanar with the orbit of Earth.[1] It was first identified as A923 PA at Heidelberg Observatory in 1923, extending the body's observation arc by 11 years prior to its official discovery observation at Johannesburg.[11]

Rotation period

In December 2010, a rotational light-curve of Limburgia was obtained from photometric observations taken by James W. Brinsfield at the Via Capote Observatory (G69) in California. It gave a rotation period of 5 hours with a brightness variation of 0.07 magnitude (U=n.a.).[9]

Diameter and albedo

According to the surveys carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Limburgia measures between 22.84 and 24.29 kilometers in diameter, and its surface has an albedo between 0.04 and 0.076.[4][5][6] In contrast, preliminary figures gave a larger diameter of 25.18 and 26.66 kilometers, respectively.[7][8] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0569 and a diameter of 22.18 kilometers using an absolute magnitude of 12.0.[3]

Naming

This minor planet was named after the Dutch province Limburg, the southernmost of the 12 provinces of the Netherlands.[2] Naming was first cited in The Names of the Minor Planets by Paul Herget in 1955 (H 125).[2]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 1383 Limburgia (1934 RV)" (2016-11-05 last obs.). Jet Propulsion Laboratory. Retrieved 11 January 2017.
  2. ^ a b c d Schmadel, Lutz D. (2007). "(1383) Limburgia". Dictionary of Minor Planet Names – (1383) Limburgia. Springer Berlin Heidelberg. p. 112. doi:10.1007/978-3-540-29925-7_1384. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f "LCDB Data for (1383) Limburgia". Asteroid Lightcurve Database (LCDB). Retrieved 11 January 2017.
  4. ^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381. Retrieved 11 January 2017.
  5. ^ a b c Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. S2CID 119293330. Retrieved 11 January 2017.
  6. ^ a b c d Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63.
  7. ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID 35447010.
  8. ^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids". The Astrophysical Journal Letters. 759 (1): 5. arXiv:1209.5794. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. S2CID 46350317. Retrieved 11 January 2017.
  9. ^ a b Brinsfield, James W. (July 2011). "Asteroid Lightcurve Analysis at the Via Capote Observatory: 1st Quarter 2011". The Minor Planet Bulletin. 38 (3): 154–155. Bibcode:2011MPBu...38..154B. ISSN 1052-8091. Retrieved 11 January 2017.
  10. ^ 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. S2CID 53493339. Retrieved 11 January 2017.
  11. ^ a b "1383 Limburgia (1934 RV)". Minor Planet Center. Retrieved 11 January 2017.

External links

This page was last edited on 25 December 2023, at 15:34
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.