comet دنبالهدار، دمدار donbâledâr (#), domdâr (#) Fr.: comète A small body of → gas and → dust
which revolves around the → Sun
in a usually very → elliptical or even
→ parabolic → orbit.
It is seen to be composed of a → head,
or → coma, and often with a spectacular gaseous
→ tail extending a great distance from the head. The rocky-icy
head is called the → comet nucleus. As the comet nears the Sun,
the increased temperature causes the → ice
in the nucleus to → sublimate and form a gaseous halo around the nucleus, called the coma. Comets often possess
two tails, a → dust tail that lies in the orbit behind
the comet generated by surface activity, and a brighter, ionized
→ gas tail, that points away from the Sun, driven by
→ solar wind. → Long-period comets are thought to originate in the → Oort cloud,
at distances exceeding 50,000 → astronomical units (AU).
They are perturbed by the planets (especially → Jupiter)
to fall in toward the Sun. Their orbits typically have random inclinations and a very large
→ eccentricity; some
→ hyperbolic orbits have been observed. → Short-period comets apparently arise in the → Kuiper belt in the zone from 20 to 50
AU. Their orbits typically have small eccentricities. Both cometary reservoirs
are thought to represent primordial solar system material. A comet
with a dust coating on its surface that inhibits gas production might be classified as an
→ asteroid. Because of this ambiguity, objects such as
→ Chiron, a → Centaur asteroid,
have been reclassified as comets. Comets are primarily composed of amorphous → water
ice, but also contain
→ carbon dioxide (CO2),
→ carbon monoxide (CO),
→ formaldehyde (H2CO),
→ methanol (CH3OH),
→ methane (CH4) at a few percent level (with
respect to water), and many other molecules at a lower level. See also
→ comet designation. Etymology (EN): From O.Fr. comète, from L. cometa, from Gk. (aster) kometes,
“long-haired (star),” from kome “hair of the head,” so called from
resemblance of the comet’s tail to streaming hair. Etymology (PE): Dombâledâr, from dombâlé “tail,” from domb, dom (Mid.Pers. dumb, Av. duma- “tail”) + -âlé, -âl resemblance suffix, → -al - dâr “having, possessor,” (from dâštan “to have, to possess,”
O.Pers./Av. root dar- “to hold, keep back, maitain, keep in mind,”
Skt. dhr-, dharma- “law,”
Gk. thronos “elevated seat, throne,”
L. firmus “firm, stable,” Lith. daryti
“to make,” PIE *dher- “to hold, support”).
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