ਮੈਗਾਪਰਸੈਕ,

megaparsec's Usage Examples:

The largest radio galaxies have lobes or plumes extending to megaparsec scales (more in the case of giant radio galaxies like 3C236), implying.

These massive, thread-like formations can reach 80 megaparsecs h−1 (or of the order of 160 to 260 million light-years) and form the.

larger scales in the universe, including kiloparsecs (kpc) for the more distant objects within and around the Milky Way, megaparsecs (Mpc) for mid-distance.

"A possible 300 megaparsec filament of clusters of galaxies in Perseus-Pegasus" 12/1985 Bibcode:1985ApJ.

(kpc) for the more distant objects within and around the Milky Way, megaparsecs (Mpc) for mid-distance galaxies, and gigaparsecs (Gpc) for many quasars.

frequently quoted in (km/s)/Mpc, thus giving the speed in km/s of a galaxy 1 megaparsec (3.

would be statistically likely for a "dead quasar" to be within a few megaparsecs of Earth.

group has an apparent radius of 200 arcseconds, and a virial radius of 1 megaparsec.

"A million cubic megaparsec void in Bootes".

Voids typically have a diameter of 10 to 100 megaparsecs (30 to 300 million light years); particularly large voids, defined by.

M87 from parsec to megaparsec scales".

However, objects beyond a megaparsec have parallax too small to be measured (the Gaia space telescope measures.

100,000 parsecs in diameter (approximately 3,000 to 300,000 light years) and are separated by distances on the order of millions of parsecs (or megaparsecs).