Event research Vesta
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Vesta at the Allas Live, Helsinki
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Vesta
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Wikipedia Bio
True color image of Vesta taken by Dawn. The massive Rheasilvia Crater dominates Vesta's south pole. | |
| Discovery | |
|---|---|
| Discovered by | Heinrich Wilhelm Olbers |
| Discovery date | 29 March 1807 |
| Designations | |
| (4) Vesta | |
| Pronunciation | /ˈvɛstə/[1] |
Named after | Vesta |
| Main belt (Vesta family) | |
| Adjectives |
|
| Symbol | |
| Orbital characteristics[6] | |
| Epoch 13 September 2023 (JD 2453300.5) | |
| Aphelion | 2.57 AU (384 million km) |
| Perihelion | 2.15 AU (322 million km) |
| 2.36 AU (353 million km) | |
| Eccentricity | 0.0894 |
| 3.63 yr (1325.86 d) | |
Average orbital speed | 19.34 km/s |
| 169.4° | |
| Inclination | 7.1422° to ecliptic 5.58° to invariable plane[7] |
| 103.71° | |
| 26 December 2021[8] | |
| 151.66° | |
| Satellites | None |
| Earth MOID | 1.14 AU (171 million km) |
| Proper orbital elements[9] | |
Proper semi-major axis | 2.36151 AU |
Proper eccentricity | 0.098758 |
Proper inclination | 6.39234° |
Proper mean motion | 99.1888 deg / yr |
Proper orbital period | 3.62944 yr (1325.654 d) |
Precession of perihelion | 36.8729 (2343 years) arcsec / yr |
Precession of the ascending node | −39.5979 (2182 years) arcsec / yr |
| Physical characteristics | |
| Dimensions | 572.6 km × 557.2 km × 446.4 km[10] |
| 525.4±0.2 km[10] | |
| Flattening | 0.2204 |
| (8.66±0.2)×105 km2[b][11] | |
| Volume | 7.4970×107 km3[10] |
| Mass | (2.590271±0.000058)×1020 kg[12] |
Mean density | 3.456±0.035 g/cm3[10] |
Equatorial surface gravity | 0.22 m/s2 (0.022 g0) |
Equatorial escape velocity | 0.36 km/s |
| 0.2226 d (5.342 h)[6][13] | |
Equatorial rotation velocity | 93.1 m/s[c] |
| 29° | |
North pole right ascension | 20h 32m[d] |
North pole declination | 48°[d] |
| 0.423[15] | |
| Temperature | min: 75 K (−198 °C) max: 250 K (−23 °C)[16] |
| V[6][17] | |
| 5.1[18] to 8.48 | |
| 3.20[6][15] | |
| 0.70″ to 0.22″ | |
Vesta (minor-planet designation: 4 Vesta) is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi).[10] It was discovered by the German astronomer Heinrich Wilhelm Matthias Olbers on 29 March 1807[6] and is named after Vesta, the virgin goddess of home and hearth from Roman mythology.[19]
Vesta is thought to be the second-largest asteroid, both by mass and by volume, after the dwarf planet Ceres.[20][21][22] Measurements give it a nominal volume only slightly larger than that of Pallas (about 5% greater), but it is 25% to 30% more massive. It constitutes an estimated 9% of the mass of the asteroid belt.[23] Vesta is the only known remaining rocky protoplanet of the kind that formed the terrestrial planets.[24] Numerous fragments of Vesta were ejected by collisions one and two billion years ago that left two enormous craters occupying much of Vesta's southern hemisphere.[25][26] Debris from these events has fallen to Earth as howardite–eucrite–diogenite (HED) meteorites, which have been a rich source of information about Vesta.[27][28][29]
Vesta is the brightest asteroid visible from Earth. It is regularly as bright as magnitude 5.1,[18] at which times it is faintly visible to the naked eye. Its maximum distance from the Sun is slightly greater than the minimum distance of Ceres from the Sun,[e] although its orbit lies entirely within that of Ceres.[30]
NASA's Dawn spacecraft entered orbit around Vesta on 16 July 2011 for a one-year exploration and left the orbit of Vesta on 5 September 2012[31] en route to its final destination, Ceres. Researchers continue to examine data collected by Dawn for additional insights into the formation and history of Vesta.[32][33]
- ^ "Vesta". Dictionary.com Unabridged (Online). n.d.
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Source: Wikipedia