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490 Veritas

From Wikipedia, the free encyclopedia
Main-belt asteroid

490 Veritas
Discovery
Discovered byMax Wolf
Discovery siteHeidelberg Obs.
Discovery date3 September 1902
Designations
(490) Veritas
Pronunciation/ˈvɛrɪtæs/[1]
1902 JP
main-belt · (outer)
Veritas[2]
AdjectivesVeritasian[3]
Orbital characteristics[4]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.37 yr (41409 d)
Aphelion3.4715 AU (519.33 Gm)
Perihelion2.8719 AU (429.63 Gm)
3.1717 AU (474.48 Gm)
Eccentricity0.094527
5.65yr (2063.2d)
31.094°
0° 10m 28.164s / day
Inclination9.2809°
178.335°
194.390°
Earth MOID1.87147 AU (279.968 Gm)
Jupiter MOID1.98443 AU (296.867 Gm)
TJupiter3.175
Physical characteristics
Dimensions110.96 ± 3.80 km[5]
115.55±5.5 km[4]
Mass(5.99 ± 2.23) × 1018 kg[5]
8.37 ± 3.23 g/cm3[5]
7.930 h (0.3304 d)
0.0622±0.006
8.53,[6] 8.32[4]

490 Veritas is a carbonaceous Veritasianasteroid, which may have been involved in one of the more massive asteroid-asteroid collisions of the past 100 million years. It was discovered by German astronomerMax Wolf atHeidelberg Observatory on 3 September 1902.

Description

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With a diameter of more than 100 kilometers, Veritas is the largest member and namesake of theVeritas family, a mid-sizedasteroid family of carbonaceous asteroids in theouter main-belt, that formed recently approximately8.5±0.5 million years ago.[2][7]: 8, 23  David Nesvorný of theSouthwest Research Institute inBoulder traced the orbits of these bodies back in time, and calculated that they formed in a collision of a body at least 150 km in diameter with a smaller asteroid. Veritas and Undina would have been the largest fragments of that collision which caused a "late Miocene dust shower". The family consists of more than a thousand known members including1086 Nata,2428 Kamenyar and2934 Aristophanes.

Late Miocene dust shower

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Substantiating Nesvorný's estimate,Kenneth Farleyet al. found evidence in sea-floor sediments of a fourfold increase in the amount ofcosmic dust reaching Earth's surface, which began 8.2 million years ago and tapered off over the next million and a half years. This is one of the largest increases in dust deposits of the past 100 million years.[8]

The suspected Veritas collision would have been too far fromJupiter for the fragments to have been slung into a collision course with Earth. However,solar radiation would have caused the resulting dust to drift inward to Earth orbit over a time span consistent with the record of dust in theocean sediment.

Today continuing collisions among Veritas-family asteroids are estimated to send five thousand tons of cosmic dust to Earth each year, 15% of the total.

Study

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490 Veritas has been observed tooccult 13 stars between 2006 and 2023.

References

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  1. ^Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^ab"Asteroid 490 Veritas – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved24 October 2019.
  3. ^James Morrow (1990)City of Truth
  4. ^abcYeomans, Donald K.,"490 Veritas",JPL Small-Body Database Browser,NASA Jet Propulsion Laboratory, retrieved9 May 2016.
  5. ^abcCarry, B. (December 2012), "Density of asteroids",Planetary and Space Science,73 (1):98–118,arXiv:1203.4336,Bibcode:2012P&SS...73...98C,doi:10.1016/j.pss.2012.03.009. See Table 1.
  6. ^Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project",The Minor Planet Bulletin,34 (4):113–119,Bibcode:2007MPBu...34..113W.
  7. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  8. ^Farley, Kenneth A.; Vokrouhlický, David; Bottke, William F.; Nesvorný, David (January 2006)."A late Miocene dust shower from the break-up of an asteroid in the main belt"(PDF).Nature.439 (7074):295–297.Bibcode:2006Natur.439..295F.doi:10.1038/nature04391.PMID 16421563. Retrieved4 September 2017.

External links

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