NGC 4247

NGC 4247

NGC 4247 is a spiral galaxy in the constellation Virgo about 182 million ly from Earth. It spans roughly 53,000 ly, about 53% of our Milky Way's width. It is receding from us at about 3,944 km/s.

Illustration from its catalogued shape, not a photograph

Spiral
type · SABa
182 million ly
from Earth · from redshift
53k ly
across
14.8
apparent magnitude
3,944 km/s
receding (RC3)

Because its light is 182 million ly from home, you are seeing NGC 4247 as it looked roughly 182 million years ago. The photons left before that much of history had passed, and are only now reaching us. This distance is estimated from the galaxy's redshift, so the lookback time is approximate.

Nearest galaxies
NGC 4297Lenticular3.4 million ly
apart
NGC 4296Lenticular4.9 million ly
apart
NGC 4246Spiral9.6 million ly
apart
IC 768Spiral17 million ly
apart
NGC 4334Spiral18 million ly
apart
NGC 4012Spiral22 million ly
apart
Worlds in the same direction on the sky

Source: structural data (position, morphology, brightness, redshift) from OpenNGC (CC BY-SA). Recession velocity from RC3 (de Vaucouleurs et al. 1991, via NASA/HEASARC, public domain). Distance computed by gravityfinder from redshift via Hubble's law (H0 = 70 km/s/Mpc).

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