Local Sheet in the context of Virgo Cluster


Local Sheet in the context of Virgo Cluster

Local Sheet Study page number 1 of 1

Play TriviaQuestions Online!

or

Skip to study material about Local Sheet in the context of "Virgo Cluster"


⭐ Core Definition: Local Sheet

The Local Sheet or the Coma–Sculptor Cloud is a nearby galaxy filament and an extragalactic region of space where the Milky Way, the members of the Local Group, and other galaxies share a similar peculiar velocity. This region lies within a diameter of about 10.4 megaparsecs (34 million light-years; 3.2×10 kilometres), 465 kiloparsecs (1.52 million light-years; 1.43×10 kilometres) thick, and galaxies beyond that distance show markedly different velocities. The Local Group has only a relatively small peculiar velocity of 66 km⋅s with respect to the Local Sheet. Typical velocity dispersion of galaxies is only 40 km⋅s in the radial direction. Nearly all nearby bright galaxies belong to the Local Sheet. The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). The Local Sheet forms a wall of galaxies delineating one boundary of the Local Void.

A significant component of the mean velocity of the galaxies in the Local Sheet appears as the result of the gravitational attraction of the Virgo Cluster of galaxies, resulting in a peculiar motion ~185 km⋅s toward the cluster. A second component is directed away from the center of the Local Void; an expanding region of space spanning an estimated 45 Mpc (150 Mly) that is only sparsely populated with galaxies. This component has a velocity of 259 km⋅s. The Local Sheet is inclined 8° from the Local Supercluster (Virgo Supercluster).

↓ Menu
HINT:

In this Dossier

Local Sheet in the context of Local Group

The Local Group is the galaxy group that includes the Milky Way, where Earth is located. It consists of two collections of galaxies in a "dumbbell" shape; the Milky Way and its satellites form one lobe, and the Andromeda Galaxy and its satellites constitute the other. The two collections are separated by about 800 kiloparsecs (3×10^ ly; 2×10 km) and are moving toward one another with a velocity of 123 km/s. The center of the group is located at about 450 kpc (1.5 million ly) away from the Milky Way, placing it slightly closer to the Andromeda Galaxy by roughly 300 kpc (1 million ly), in which the latter may be more massive than the former in terms of mass.

The Local Group has a total mass of the order of 2×10 solar masses (4×10 kg), and also a total diameter of 5.11 megaparsecs (17 million light-years; 1.6×10 kilometres) based on density matching and the potential surface of its parent structure, Local Sheet. It is itself a part of the Local Volume and the larger Virgo Supercluster, which is a part of the even greater Laniakea Supercluster along with the Pisces–Cetus Supercluster Complex. The exact number of galaxies in the Local Group is unknown, as the Milky Way obscures some; however, a current total of 134 members is known within 1 megaparsec from the center, most of which are dwarf galaxies. The Local Group was thought to have been more spread in the early universe with 7 megaparsecs (23 million light-years; 2.2×10 kilometres) by 700 million years after the Big Bang.

View the full Wikipedia page for Local Group
↑ Return to Menu