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

From Wikipedia, the free encyclopedia

138 Tolosa
3D convex shape model of 138 Tolosa
Discovery
Discovered byHenri Joseph Perrotin
Discovery date19 May 1874
Designations
(138) Tolosa
Pronunciation/tˈlsə/[1][2]
Named after
Toulouse (Tolōsa)
A874 KA; 1909 SB
Main belt
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc110.38 yr (40315 d)
Aphelion2.8463 AU (425.80 Gm)
Perihelion2.05145 AU (306.893 Gm)
2.44887 AU (366.346 Gm)
Eccentricity0.16229
3.83 yr (1399.7 d)
18.91 km/s
348.297°
0° 15m 25.884s / day
Inclination3.2038°
54.762°
260.825°
Physical characteristics
Dimensions51.86 ± 3.07 km[4]
45.50±2.1 km[3][5]
Mass(4.93 ± 2.59) × 1017 kg[4]
Mean density
6.74 ± 3.74 g/cm3[4]
Equatorial surface gravity
0.0127 m/s²
0.0241 km/s
10.101 h (0.4209 d)[3]
10.103 h[5]
0.2699±0.027[3][5]
Temperature~178 K
S
8.75

Tolosa (minor planet designation: 138 Tolosa) is a brightly coloured, stony background asteroid from the inner region of the asteroid belt. It was discovered by French astronomer Henri Joseph Perrotin on 19 May 1874, and named by the Latin and Occitan name ([tɔˈloːsa] and [tuˈluzɔ]) of the French city of Toulouse.

The spectrum of this asteroid rules out the presence of ordinary chondrites, while leaning in favor of clinopyroxene phases. As of 2006, there are no known meteorites with compositions similar to the spectrum of 138 Tolosa.[5]

References

  1. ^ Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  2. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  3. ^ a b c d Yeomans, Donald K., "138 Tolosa", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016.
  4. ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
  5. ^ a b c d Hardersen, Paul S.; et al. (March 2006), "Near-infrared spectral observations and interpretations for S-asteroids 138 Tolosa, 306 Unitas, 346 Hermentaria, and 480 Hansa" (PDF), Icarus, vol. 181, no. 1, pp. 94–106, Bibcode:2006Icar..181...94H, doi:10.1016/j.icarus.2005.10.003, archived from the original (PDF) on 10 August 2017, retrieved 30 March 2013.

External links


This page was last edited on 25 December 2023, at 14:56
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.