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895 Helio

From Wikipedia, the free encyclopedia
Main-belt asteroid

895 Helio
Discovery
Discovered byMax Wolf
Discovery siteHeidelberg
Discovery date11 July 1918
Designations
(895) Helio
Pronunciation/ˈhli/[1]
1918 DU
AdjectivesHelian/ˈhliən/
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc109.79 yr (40100 days)
Aphelion3.6686 AU (548.81 Gm)
Perihelion2.7362 AU (409.33 Gm)
3.2024 AU (479.07 Gm)
Eccentricity0.14558
5.73yr (2093.2d)
241.229°
0° 10m 19.164s / day
Inclination26.077°
264.704°
178.108°
Earth MOID1.75069 AU (261.899 Gm)
Jupiter MOID1.60187 AU (239.636 Gm)
TJupiter3.019
Physical characteristics
148.43 ± 5.02 km[3]
109.568±1.987km[2]
Mass(9.87 ± 6.05) × 1018 kg[3]
5.76 ± 3.58 g/cm3[3]
9.3959 h (0.39150 d)
9.3959 h[2]
0.0420±0.002[2]
FCB/B[2]
8.3[2]

895 Helio is a large dark outermain-beltasteroid[4] about 150 km in diameter. It was discovered on 11 July 1918 by German astronomerMax Wolf.[2] It is named after the elementhelium, whose spectrum was studied byFriedrich Paschen andCarl David Tolmé Runge, with the asteroid being named by Paschen at Wolf's request; the namehelium itself comes fromHelios, theGreek god of theSun.

This is aB-type asteroid.[2] The best spectral analog for 895 Heloi is the iron richpyroxene mineralhedenbergite. It shares similar orbital properties with the31 Euphrosyneasteroid family, but is most likely an interloper.[5]Light curve analysis provides a rotation period of 9.4 hours.[4]

References

[edit]
  1. ^"helio".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  2. ^abcdefgh"JPL Small-Body Database Browser: 895 Helio".Jet Propulsion Laboratory. Retrieved3 May 2016.
  3. ^abcCarry, 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.
  4. ^abPolakis, Tom; Skiff, Brian A. (October 2016), "Lightcurve Analysis for Asteroids 895 Helio and 1108 Demeter",Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers,43 (4): 310,Bibcode:2016MPBu...43..310P.
  5. ^Yang, B.; et al. (November 2020), "Physical and dynamical characterization of the Euphrosyne asteroid family",Astronomy & Astrophysics,643: 9,arXiv:2009.04489,Bibcode:2020A&A...643A..38Y,doi:10.1051/0004-6361/202038567, A38

External links

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