Based on a recessional velocity of 2375 km/sec, NGC 4200 is about 110 million light years away. Given that and its apparent size of 1.5 by 0.9 arcmin, it is about 50 thousand light years across.

The second IC lists a corrected RA (per Howe) of 12 07 31.

The 700 km/sec recessional velocity of NGC 4206 is too small in comparison with peculiar (non-Hubble expansion) velocities to provide a reliable distance estimate. Redshift-independent distance estimates of 55 to 75 million light years are therefore considered more likely to be correct than the much smaller 30 million light year distance obtained from the recessional velocity. Presuming an actual distance of 65 million light years, its apparent size of 5.2 by 0.75 arcmin suggests that the galaxy is about 100 thousand light years across. Given its probable distance, NGC 4206 is probably a member of the Virgo Cluster of galaxies.

The first IC notes "Not seen by Spitaler, to be struck out".

An all too frequent duplicate observation, made unusual by being on the same night, but still not unique.

The 130 km/sec recessional velocity of NGC 4216 is far too small in comparison to peculiar (non-Hubble expansion) velocities to provide a reliable distance estimate. Redshift-independent distance estimates range from 45 to 65 million light years, indicating that it is a member of the Virgo Cluster. Using a probable distance of 55 million light years and its apparent size of 8.1 by 1.8 arcmin suggests the galaxy is about 130 thousand light years across.

The 230 km/sec recessional velocity of NGC 4222 is far too small, in comparison to peculiar (non-Hubble expansion) velocities, to provide a reliable distance estimate. Redshift-independent distance estimates are around 70 million light years, indicating that it is a member of the Virgo Cluster. Given that and its apparent size of 3.2 by 0.45 arcmin, the galaxy is about 65 thousand light years across.

The 735 km/sec recessional velocity of NGC 4241 is too small, in comparison to peculiar (non-Hubble expansion) velocities, to provide a reliable distance estimate. Redshift-independent distance estimates of 50 to 75 million light years are undoubtedly more reliable than the 35 million light year distance obtained from the recessional velocity, and suggest that it is a member of the Virgo Cluster. Using an "average" distance of 65 million light years, the galaxy's apparent size of 2.0 by 2.0 arcmin suggests that it is about 40 thousand light years across. Note: Entering NGC 4241 in the Wikisky database shows NGC 4223; to see the correct galaxy, use the IC or PGC number.