Search results
Results From The WOW.Com Content Network
Nonetheless, collisions between large asteroids occur and can produce an asteroid family, whose members have similar orbital characteristics and compositions. Individual asteroids within the belt are categorized by their spectra, with most falling into three basic groups: carbonaceous , silicate , and metal-rich .
Asteroids are classified by their characteristic emission spectra, with the majority falling into three main groups: C-type, M-type, and S-type. These describe carbonaceous (carbon-rich), metallic, and silicaceous (stony) compositions, respectively. The physical composition of asteroids is varied and in most cases poorly understood.
Main-belt asteroids have orbital elements constrained by ... asteroids located in Jupiter's L 4 and L 5 Lagrange ... Most mass values of asteroids are assumed. [123 ...
These asteroids are in stable 2:1 libration with Jupiter, in high-inclination orbits. There are about 5 to 10 of these known so far, with 1362 Griqua and 8373 Stephengould the most prominent. The Cybele asteroids have a mean orbital radius between 3.27 AU and 3.7 AU, [3] an eccentricity less than 0.3, [4] and an inclination less than 30°. [3]
Asteroids are given minor planet numbers, but not all minor planets are asteroids. Minor planet numbers are also given to objects of the Kuiper belt , which is similar to the asteroid belt but farther out (around 30–60 AU), whereas asteroids are mostly between 2–3 AU from the Sun or at the orbit of Jupiter 5 AU from the Sun.
The Hilda asteroids (adj. Hildian) are a dynamical group of more than 6,000 asteroids located beyond the asteroid belt but within Jupiter's orbit, in a 3:2 orbital resonance with Jupiter. [ 1 ] [ 2 ] The namesake is the asteroid 153 Hilda .
Most asteroids are located in the asteroid belt, between Mars and Jupiter. This is a cold region, with temperatures ranging from –73 °C to –103 °C. [31] Human life will require a consistent energy source for warmth.
For example, there are very few asteroids with semimajor axis near 2.50 AU, period 3.95 years, which would make three orbits for each orbit of Jupiter (hence, called the 3:1 orbital resonance). Other orbital resonances correspond to orbital periods whose lengths are simple fractions of Jupiter's.