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The Intergalactic Wanderer (NGC 2419)
Globular Cluster
aka NGC 2419
RA: 07h38m08.0s, Dec: +38°52'54" (2000) in Lynx
Magnitude: 10.3
Size: 4.6'
Distance: 200000 ly

Minimum requirements to detect: 8-inch telescope

NGC 2419 is a small globular cluster in Lynx. It lies some 200,000 light years away, which accounts for how small and faint it is. It is some ten times farther away than the famous M13, for instance. To add another perspective, this cluster lies nearly twice as far away from the galactic center as the Large Magellanic Cloud! The vast majority of globulars lie less than 1/3 as far out.

This may be the most distant Milky Way globular visible in amateur instruments.


This image from the DSS shows a 20' x 20' field. North is down and east is to the right.

NGC 2419 was discovered by William Herschel in 1788. He and later observers failed to note its globular nature. In smaller (<10-inch) telescopes it appears as a small, round hazy ball. Larger apertures begin to resolve individual stars.

It is an easy find because two 7th magnitude stars (visible in most finders) point directly at it. In my 18-inch it appeared as a round haze at 100x. My best view was at 425x, where many individual stars were resolved.


The field in a 6-inch at 50x.

Millennium Star Atlas Vol I Chart 107
Sky Atlas 2000 Chart 5
Uranometria 2000 Vol I Chart 100
Uranometria 2nd Ed. Chart 57
Herald-Bobroff Astroatlas B-11 C-33