Dark Comet
20-12-2024
09:31 AM
1 min read
Overview:
NASA scientists are closely studying a new class of celestial objects known as “dark comets”.
About Dark Comet:
- They are celestial bodies which lack the glowing tails and resemble asteroids.
- The first indication of dark comets came in 2016, when asteroid 2003 RM exhibited unusual orbital deviations.
- Since then, astronomers have confirmed the existence of dark comets, with a new study published which revealed 14 such objects.
- These comets fall into two main categories: “outer dark comets,” which have eccentric orbits and are larger, and “inner dark comets,” which are smaller and closer to the Sun, with nearly circular orbits.
- Dark comets are often small, just a few metres to a few hundred metres wide.
- They have less surface area for material to escape and form into the beautiful tails we see on typical comets.
- They often spin quite rapidly and disperse escaping gas and dust in all directions, making them less visible.
- They follow elongated, elliptical paths that bring them close to the Sun before sweeping back out to the farthest reaches of the Solar System.
Q1: What are Asteroids?
Asteroids, sometimes called minor planets, are rocky remnants left over from the earlyformation of our solar system about 4.6 billion years ago.
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