Local Sheet

The Local Sheet in astronomy is a nearby extragalactic region of space where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 7001660000000000000♠ 66 km⋅s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies is only 7001400000000000000♠ 40 km⋅s ⁻¹ in the radial direction. ^[2] Nearly all nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4] The Local Sheet forms a wall of galaxies delineating one boundary of the Local Void . ^[5]

Page Revisions

Year	Metadata	Sections	Top Words	First Paragraph
2018	38660 characters 2 sections 4 paragraphs 11 images 80 internal links 14 external links	1. See also 2. References	galaxies 0.493 local 0.405 mly 0.350 sheet 0.265 mpc 0.233 ellipticals 0.194 peculiar 0.166 velocity 0.163 supercluster 0.130 component 0.101 7002185000000000000 0.097 7002259000000000000 0.097 logarithm 0.097 maffei 0.097 virgo 0.097	The Local Sheet in astronomy is a nearby extragalactic region of space where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 7001660000000000000♠ 66 km⋅s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies is only 7001400000000000000♠ 40 km⋅s ⁻¹ in the radial direction. ^[2] Nearly all nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4] The Local Sheet forms a wall of galaxies delineating one boundary of the Local Void . ^[5]
2017	26397 characters 1 sections 4 paragraphs 1 images 74 internal links 11 external links	1. References	galaxies 0.459 local 0.402 mly 0.367 sheet 0.278 mpc 0.244 ellipticals 0.203 peculiar 0.174 velocity 0.171 supercluster 0.136 component 0.106 7002185000000000000 0.102 7002259000000000000 0.102 logarithm 0.102 maffei 0.102 virgo 0.101	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 7001660000000000000♠ 66 km⋅s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 7001400000000000000♠ 40 km⋅s ⁻¹ in the radial direction. ^[2] All nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4]
2016	26251 characters 1 sections 4 paragraphs 1 images 72 internal links 11 external links	1. References	galaxies 0.459 local 0.402 mly 0.367 sheet 0.278 mpc 0.244 ellipticals 0.203 peculiar 0.174 velocity 0.171 supercluster 0.136 component 0.106 7002185000000000000 0.102 7002259000000000000 0.102 logarithm 0.102 maffei 0.102 virgo 0.101	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 7001660000000000000♠ 66 km⋅s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 7001400000000000000♠ 40 km⋅s ⁻¹ in the radial direction. ^[2] All nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4]
2015	25489 characters 1 sections 4 paragraphs 1 images 71 internal links 11 external links	1. References	galaxies 0.468 local 0.410 mly 0.374 sheet 0.283 mpc 0.249 ellipticals 0.207 peculiar 0.177 velocity 0.174 supercluster 0.139 component 0.108 log 0.104 maffei 0.104 virgo 0.103 cluster 0.100 spirals 0.080	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 66 km s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 40 km s ⁻¹ in the radial direction. ^[2] All nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4]
2014	22660 characters 1 sections 3 paragraphs 1 images 51 internal links 11 external links	1. References	galaxies 0.475 local 0.416 mly 0.380 sheet 0.288 mpc 0.253 ellipticals 0.210 peculiar 0.180 velocity 0.177 supercluster 0.141 component 0.110 virgo 0.105 cluster 0.102 spirals 0.081 outlines 0.081 group 0.080	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[2] This region lies within a radius of about 7 Mpc (23 Mly ), ^[3] 0.46 Mpc (1.5 Mly) thick, ^[1] and galaxies beyond that distance show markedly different velocities. ^[3] The Local Group has only a relatively small peculiar velocity of 66 km s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 40 km s ⁻¹ in the radial direction. ^[2] All nearby bright galaxies belong to the Local Sheet. ^[1] The Local Sheet is part of the Local Volume and is in the Virgo Supercluster (Local Supercluster). ^[4]
2013	9322 characters 1 sections 2 paragraphs 0 images 13 internal links 6 external links	1. References	galaxies 0.603 peculiar 0.305 velocity 0.299 local 0.274 sheet 0.216 mpc 0.214 component 0.185 cluster 0.172 dispersion 0.129 markedly 0.123 259 0.123 sparsely 0.114 185 0.102 attraction 0.100 populated 0.099	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[1] This region lies within a radius of about 7 Mpc , and galaxies beyond that distance show markedly different velocities. ^[2] The Local Group has only a relatively small peculiar velocity of 66 km s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 40 km s ⁻¹ in the radial direction. ^[1]
2012	9322 characters 1 sections 2 paragraphs 0 images 13 internal links 6 external links	1. References	galaxies 0.603 peculiar 0.305 velocity 0.299 local 0.274 sheet 0.216 mpc 0.214 component 0.185 cluster 0.172 dispersion 0.129 markedly 0.123 259 0.123 sparsely 0.114 185 0.102 attraction 0.100 populated 0.099	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[1] This region lies within a radius of about 7 Mpc , and galaxies beyond that distance show markedly different velocities. ^[2] The Local Group has only a relatively small peculiar velocity of 66 km s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 40 km s ⁻¹ in the radial direction. ^[1]
2011	9419 characters 1 sections 2 paragraphs 0 images 12 internal links 4 external links	1. References	galaxies 0.603 peculiar 0.305 velocity 0.299 local 0.274 sheet 0.216 mpc 0.214 component 0.185 cluster 0.172 dispersion 0.129 markedly 0.123 259 0.123 sparsely 0.114 185 0.102 attraction 0.100 populated 0.099	The Local Sheet in astronomy is a nearby region of the observable universe where the Milky Way , the members of the Local Group and other galaxies share a similar peculiar velocity . ^[1] This region lies within a radius of about 7 Mpc , and galaxies beyond that distance show markedly different velocities. ^[2] The Local Group has only a relatively small peculiar velocity of 66 km s ⁻¹ with respect to the Local Sheet. Typical velocity dispersion of galaxies within the Local Sheet is only 40 km s ⁻¹ in the radial direction. ^[1]