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4 VESTA

Asteroid


Actual
Compared
to Earth
Age ~ 4.5 billion years about the same age as the Sun
Actual Brightness -- --
Location Solar system, asteroid belt --
Avg. Distance
from the Sun
220 million miles 2.4
Diameter 330 miles 0.04
Mass 3 x 1020 kg --
Density (gram/cubic cm) -- --
Orbital Period
around the Sun
3.6 Earth years 3.6
Rotation Period 5.3 hours 3.6
Surface Gravity -- --
Surface Temperature (average) -- --
Number of moons 0 --

What To Look For Through The Telescope


  1. Recommended eyepiece: 26mm or 40 mm.

  2. Vesta resembles a star through the telescope. It is about the same brightness as Saturn’s moon Titan and a bit dimmer than Jupiter’s four Galilean moons. Vesta has an orange tint.


4 Vesta Information


  1. Vesta is the fourth asteroid ever discovered, thus the name “4 Vesta.” It was discovered by H.W. Olbers in 1807. It is the third largest asteroid in the asteroid belt, and it is the only asteroid that can be seen with the unaided eye (under very favorable viewing locations).

  2. Vesta is a very interesting asteroid.

    a. Vesta is the most geologically diverse of the large asteroids, and the only one known with distinct light and dark areas.

    b. Lava flows are found on the asteroid.

    c. One impact crater is so deep it exposes the asteroid’s subsurface, or mantle.

  3. The light and dark areas on the asteroid correspond to different layers of the asteroid. This means the asteroid “differentiated” into layers long ago, like the terrestrial planets Mercury, Venus, Earth, and Mars.

    a. First, start with an object in space, for example, the Earth.

    b. Several different types of material with different densities are found in this object.

    c. If the object is very, very hot, these materials melt.

    d. Molten, more dense material sinks towards the center of the object while the molten, less dense material stays near the surface.

    e. Differentiation can only occur if the object is very hot, otherwise, the dense materials would not melt and could not sink.

    f. Long ago, Earth was very, very hot. Molten iron sunk to the core of Earth, while less dense materials stayed near the surface.

    g. Since Vesta is differentiated, it means Vesta was once very hot.

  4. Two fence workers in Millbillillie, Western Australia, saw a fireball headed towards the ground in October, 1960. Ten years later, pieces of the fallen meteorite were found.

  5. Signatures in the spectra (of light reflected off the surface) of the meteorite matches signatures in the spectra (of sunlight reflected off the surface) of Vesta: the meteorite is from Vesta.

  6. Other small asteroids have recently been discovered near Vesta that have the same spectral signature as Vesta and the meteorite. These asteroids are considered chips blasted off of Vesta’s surface.

  7. Other meteorites on Earth are probably from Vesta: they just haven’t been found or identified yet.

Home > Solar System > Asteroids > 4 Vesta > References top
References
Item Updated Notes
Updated “View through telescope” info 2003-03-21
Distance from Sun 2017-04-305 http://amazingspace.org/resource_page/79/solar_system/type#resource_tab
Revolution Period 2017-04-30 http://amazingspace.org/resource_page/79/solar_system/type#resource_tab
Rotation Period 2003-02-05 http://nssdc.gsfc.nasa.gov/planetary/factsheet/asteroidfact.html
Diameter 2017-04-30 http://amazingspace.org/resource_page/79/solar_system/type#resource_tab
http://www.solarviews.com/eng/vesta.htm
Mass 2017-04-30 http://amazingspace.org/resource_page/79/solar_system/type#resource_tab
Surface Gravity --
Temperature --
Density --
Other Information 2003-02-05 University of Cambridge’s Institute for Astronomy
http://www.ast.cam.ac.uk/HST/press/vestamap.html
Sites given above for other details
http://www.hohmanntransfer.com/cat/a4.htm