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.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
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

(613100) 2005 TN74

From Wikipedia, the free encyclopedia

(613100) 2005 TN74
Discovery
Discovered byScott S. Sheppard, Chad Trujillo
Discovery date8 October 2005
Designations
2005 TN74
3:5 resonant TNO
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 4
Observation arc1805 days (4.94 yr)
Aphelion52.49343 AU (7.852905 Tm)
Perihelion32.11131 AU (4.803784 Tm)
42.30237 AU (6.328344 Tm)
Eccentricity0.24091
275.14 yr (100495 d)
351.03607°
0° 0m 12.896s /day
Inclination2.17385°
179.25692°
224.79728°
Earth MOID31.1197 AU (4.65544 Tm)
Jupiter MOID27.1241 AU (4.05771 Tm)
Physical characteristics
Dimensions85–240 km
7.3[1]

(613100) 2005 TN74 (provisional designation 2005 TN74) is a trans-Neptunian object (TNO)[2] in a 3:5 resonance with Neptune.[3][4] It was discovered by Scott S. Sheppard and Chadwick A. Trujillo in 2005.

It was initially suspected of being a Neptune trojan since the first observations gave it a semi-major axis of 30 AU and an orbital eccentricity of 0.16,[5] but further observations showed it to have a semi-major axis of 42.7 AU, a perihelion of 32.1 AU, and an aphelion of 53.4 AU.[1]

With an absolute magnitude of 7.2,[1] it has an expected diameter in the range of 85 to 240 km.[6]

It has been observed 19 times over four oppositions.[1]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 2005 TN74". Retrieved 30 March 2016.
  2. ^ Most SDOs have a perihelion distance greater than 35AU and an eccentricity of more than 0.3.
  3. ^ "Orbit Fit and Astrometric record for 05TN74". Archived from the original on 29 April 2018. Retrieved 7 March 2012.
  4. ^ Wasserman, L. H.; Buie, M. W.; Marsden, B. G. (5 October 2006). "MPEC 2006-T35 : 2005 PR21, 2005 PT21, 2005 PU21, 2005 TN74". Minor Planet Center. Retrieved 12 May 2008.
  5. ^ Sheppard, S. S.; Trujillo, C. A.; Marsden, B. G. (31 October 2005). "MPEC 2005-U97 : 2005 TN74, 2005 TO74". Minor Planet Center. Retrieved 12 May 2008.
  6. ^ "Absolute Magnitude (H)". Archived from the original on 2 March 2001. Retrieved 11 May 2008.

External links

This page was last edited on 18 January 2024, at 20:33
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.