There is something about capturing multiple galaxies within a single eyepiece field that boggles the mind. Our own galaxy, the Milky Way, completely surrounds us. If Earth's orbital path about the Sun were scaled down to a circle one-inch across, the Milky Way would still be more than 60,000 miles across. It is asking a lot to accept that something so large can appear so fragile and insignificant when viewed through a telescope. To present two or more of these behemoths within a single eyepiece field staggers the imagination.
Autumn Sky Tour: NGC 584 and NGC 596 (Cetus) RA: 01h 32.2m / DEC: -06° 57'.0 |
NGC 584 and NGC 596 are among several fine galaxy groupings in Cetus. Cetus, the sea monster, is one of the largest constellations by area. The head is defined by a pentagonal arrangement of stars near the southeast corner of Pisces. The body of the seamonster is separated from the head by nearly 20 degrees. All the stars in the body should be at naked eye visibility under a dark sky. However, none is brighter than about 4th magnitude and that makes Cetus a challenging constellation to identify.
NGCs 584 and 596 form a nice pair at low power. The sketch at left captures the view at 82X (Meade 13.8-mm SWA) in my 10-inch Starfinder Newtonian. 10.5 magnitude NGC 584 is listed as a loosely structured spiral or early lenticular galaxy in Uranometria. It covers a 2'x1' areaa in the 10-inch. NGC 596 as a 10.9 magnitude lenticular, similar in size to NGC 584, positioned 24' to the southeast. Moderate aperture will reveal NGC 586 just a few arc minutes east of NGC 584. NGC 586 is a 13.2 magnitude lenticular galaxy. If you find it, then try for nearby NGC 600 and NGC 615. After completing this tour, take a moment to contemplate the fact that you have just observed several hundred-billion stellar population galaxies within this very small scrap of sky. |
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Revised: March 6, 2002 [WDF]