About Solar cloud system
The cloud is thought to encompass two regions: a disc-shaped inner Oort cloud aligned with the solar ecliptic (also called its Hills cloud) and a spherical outer Oort cloud enclosing the entire Solar System.
The Oort cloud ,sometimes called the Öpik–Oort cloud,isto be a cloud of billions of surrounding theat distances ranging from 2,000 to 200,000(0.03 to 3.2 ). Its existence was proposed in 1950 by.
The Oort cloud is thought to occupy a vast space somewhere between 2,000 and 5,000 AU (0.03 and 0.08 ly)from the Sun to as far out as 50,000 AU (0.79 ly) or even 100,000 to 200,000 AU (1.58 to 3.16 ly). The region can be subdivided into a spherical outer Oort cloud with a radius of.
are remnants from the formation of the Solar system around 4 billion years ago, stored in two separate areas, theand the Oort cloud.Short-period comets (those with orbits of up to 200 years) are generally accepted to have emerged from either the Kuiper belt.
Most of the comets seen close to the Sun seem to have reached their current positions through gravitational perturbation of the Oort cloud by theexerted by the . Just as the 's tidal force deforms Earth's oceans, causing the tides to rise and fall, the galactic tide.
By the early 20th century, astronomers had identified two main types of comets: short-period comets (also calledcomets) and long-period comets (also called nearlycomets).Ecliptic comets have relatively small orbits aligned near theand.
The Oort cloud is thought to have developed after thefrom the primordialapproximately 4.6 billion years ago.The most widely accepted hypothesis is that the Oort cloud's objects initially coalesced much closer to the Sun as part of the.
Several observed objects have been proposed as members of the inner Oort cloud.Sedna, first reported in 2004, has a highly eccentric orbit with a perihelion distances of 76 AU., observed in 2012, has a larger perihelion (closest approach to the Sun) but its aphelion is.
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