Luminous Galaxies Within 57 Mly
All (total of 427) galaxies within 57 million light years (Mly) with an absolute B magnitude less than -18.4 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 54.7 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid. The few labeled galaxies are galaxies in the Messier catalog (Other galaxies are labeled in the additional views below by subsets of absolute magnitude).
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Less Than -21
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -21.0 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 36.5 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -20.5 and -21
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -20.5 but greater than or equal to -21 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 40.6 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -20.2 and -20.5
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -20.2 but greater than or equal to -20.5 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 41.1 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -19.9 and -20.2
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -19.9 but greater than or equal to -20.2 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 54.7 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -19.7 and -19.9
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -19.7 but greater than or equal to -19.9 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 43.4 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -19.5 and -19.7
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -19.5 but greater than or equal to -19.7 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 42.0 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -19.3 and -19.5
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -19.3 but greater than or equal to -19.5 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 47.2 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -19.1 and -19.3
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -19.1 but greater than or equal to -19.3 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 37.6 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -18.9 and -19.1
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -18.9 but greater than or equal to -19.1 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 38.7 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -18.7 and -18.9
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -18.7 but greater than or equal to -18.9 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 38.6 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -18.55 And -18.7
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -18.55 but greater than or equal to -18.7 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 39.4 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Subset View: Luminous Galaxies Within 57 Mly, With Absolute B Magnitude Between -18.4 and -18.55
The subset of galaxies within 57 million light years (Mly) with an absolute B magnitude less than -18.4 but greater than or equal to -18.55 (the more negative the absolute magnitude, the more luminous, the more intrinsically bright the galaxy. The absolute magnitude of the Milky Way galaxy is estimated to be -20.8). Data is from: The 50 Mpc Galaxy Catalog (50 MGC): Consistent and Homogeneous Masses, Distances, Colors, and Morphologies. David Ohlson, Anil C. Seth, Elena Gallo, Vivienne F. Baldassare, and Jenny E. Greene, The Astronomical Journal, 167:31 (18pp), 2024 January. Cutoff at 57 million light years (Mly) takes us into the Virgo Cluster (visible as the cluster of galaxies near the end of the "To Virgo Cluster" axis). The base grid parallels the supergalactic plane, and lies 43.4 million light years (Mly) below the actual supergalactic plane. The actual supergalactic plane is visible as the second grid above the base grid.
Click here for a table of the data used to generate this view.
Beyond Our Galaxy
