NGC 488

At an estimated distance of 90 million light years away NGC 488 is an intriguing galaxy despite its distance from us. This galaxy displays subtle and tightly wound blue spiral arms with a yellowish core. Astronomers that have recently observed this galaxy note that the stars in the disk are orbiting the galaxy at a break-neck speed of 360km/s. If this number seems large to you- bear in mind you are orbiting the center of the Milky Way at 220 km/s. By studying the velocity distribution of stars in a galaxy like this astronomers attempt to answer fundamental questions concerning the structure of spiral galaxies. For example, observations of this galaxy confirm that it is the process of star formation (molecular clouds) and not the kinematic motions of stars that determine the spiral appearance of spiral galaxies. Other galaxies similar to NGC 488 include NGC 2841 and NGC 7217.

This image was taken as part of Advanced Observing Program (AOP) program at Kitt Peak Visitor Center during 2014.

Credit:

KPNO/NOIRLab/NSF/AURA/Tony Kriz/Adam Block

About the Image

Id:noao-n488kriz
Type:Observation
Release date:Feb. 25, 2014, 12:29 p.m.
Size:1200 x 809 px

About the Object

Name:NGC 4889
Constellation:Pisces
Category:Galaxies

Image Formats

Large JPEGLarge JPEG
181.5 KB
Screensize JPEGScreensize JPEG
100.0 KB

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Coordinates

ObjectValue
Position (RA):1 21 37.32
Position (Dec):5° 14' 59.09"
Field of view:14.30 x 9.63 arcminutes
Orientation:North is 86.9° right of vertical


Colors & filters

BandWave-lengthTele-scope
Optical
B
438 nmVisitor Center 0.4-meter Telescope
Other CCD
Optical
G
475 nmVisitor Center 0.4-meter Telescope
Other CCD
Optical
R
625 nmVisitor Center 0.4-meter Telescope
Other CCD
Optical
Broad Band
555 nmVisitor Center 0.4-meter Telescope
Other CCD