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Galaxy · Spiral

UGC 7751

UGC 7751 is a galaxy in the direction of the constellation Canes Venatici, 25.8 million light-years away.

TypeSpiral
ConstellationCanes Venatici
Distance25.8 million light-years (7.90 Mpc)
Diameter8,937 light-years · 0.1 × the Milky Way
Absolute magnitudemagnitude −13.70
Apparent magnitudemagnitude 15.79
Luminosity0.0013 × the Milky Way
Right ascension (J2000)12h 35m 11.8s
Declination (J2000)+41° 03′ 39″
SourceUpdated Nearby Galaxy Catalog (Karachentsev et al. 2013)

In the sky

A telescope is needed to see it: its apparent magnitude is 15.79. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out 26 million years ago. At that time the dinosaurs were gone and mammals were diversifying; there was no human lineage yet. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 457.1 billion years.

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