Scale at Hubble Flow Distances |
Type | Values |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
Cosmology-Corrected Quantities [H0 = km/sec/Mpc, Ωmatter = , Ωvacuum = ] |
[Redshift as corrected to the Reference Frame defined by the ] |
Type | Values |
| Mpc (m-M) = mag |
| Mpc (m-M) = mag |
| Mpc (m-M) = mag |
| Mpc (m-M) = mag |
| Gpc^3 |
| Gyr |
| Gyr |
| Gyr |
| pc/arcsec = kpc/arcsec = kpc/arcmin = Mpc/degree |
| Flux Density per Unit Area = ; Magnitude per Unit Area = mag |