
NGC 280 - Wikipedia
NGC 280 is a spiral galaxy in the constellation Andromeda. It was discovered on December 5, 1785 by William Herschel. [2]
NGC 280 - Intermediate Spiral Galaxy in Pisces | TheSkyLive.com
NGC 280 is a Intermediate Spiral Galaxy in the Pisces constellation. NGC 280 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year.
NGC 280 Galaxy Facts (UGC 534) & Distance - Universe Guide
NGC 280 is a Spiral Galaxy located in the constellation of Andromeda in the northern hemisphere. NGC 280's distance from Earth is 409,877,458.28 light years. NGC 280 is called NGC 280 in the New General Catalogue (NGC). This catalogue is a list of deep space objects compiled by John Louis Emil Dreyer in 1888 to update John Herschel's earlier work.
NGC280 (Galaxy) - In-The-Sky.org
Click and drag the chart above to pan around the sky, or use the mouse wheel to zoom. Click to enlarge. From Virginia Beach , NGC280 will become visible at around 18:20 (EST), 67° above your south-western horizon, as dusk fades to darkness. It will then sink towards the horizon, setting at 00:16.
NGC 280 | galaxy in Andromeda | New General Catalogue
< NGC List NGC 280. NGC 280 is a mixed spiral galaxy located in the constellation of Andromeda. The NGC is a catalog of 7,840 nebulae, star clusters, and galaxies. Here are the key stats on NGC 280:
NGC 280 - Wikiwand
NGC 280 is a spiral galaxy in the constellation Andromeda. It was discovered on December 5, 1785 by William Herschel.
Category:NGC 280 - Wikimedia Commons
The following 2 files are in this category, out of 2 total.
NGC 280 (H80) in Andromeda | Herschel Catalogue
NGC 280 (H80) NGC 280 (H80) is a galaxy located in the constellation of Andromeda. The Herchel 2500 is a catalog of nebulae, star clusters, and galaxies. Here are the key stats on NGC 280:
Galaxy NGC 280 - Galaxy in Andromeda Constellation
Pictures, altitude charts, data sheet and sky map for NGC 280 - Galaxy in Andromeda Constellation
NGC 280 - Galaxy - SKY-MAP
Rotational Widths for Use in the Tully-Fisher Relation. I. Long-Slit Spectroscopic Data We present new long-slit Hα spectroscopy for 403 noninteractingspiral galaxies, obtained at the Palomar Observatory 5 m Hale telescope,which is used to derive well-sampled optical rotation curves.
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