File:UGC 9391 - HST - Heic1611c.tif

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	21:44, 1 April 2020		2,800 × 2,800 (19.71 MB)	commons>Fabian RRRR	== {{int:filedesc}} == {{Information \|Description='''UGC 9391 Cepheid variable stars in this spiral galaxy, known as UGC 9391, and a Type Ia supernova (not visible in this image) were used by a team of astronomers to calculate the expansion rate of the modern Universe. Credit: NASA, ESA, and L. Frattare (STScI) Coordinates Position (RA): 14 34 36.70 Position (Dec): 59° 20' 12.75" Field of view: 1.85 x 1.85 arcminutes Orientation: North is 16.8° left of vertical Colours & fil...

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Image title	Cepheid variable stars in this spiral galaxy, known as UGC 9391, and a Type Ia supernova (not visible in this image) were used by a team of astronomers to calculate the expansion rate of the modern Universe.
Width	2,800 px
Height	2,800 px
Bits per component	8 8 8
Compression scheme	LZW
Pixel composition	RGB
Orientation	Normal
Number of components	3
Number of rows per strip	31
Horizontal resolution	300 dpi
Vertical resolution	300 dpi
Data arrangement	chunky format
Software used	Adobe Photoshop CC 2015 (Macintosh)
File change date and time	13:16, 1 June 2016
Color space	sRGB