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File:UGC 9391 - HST - Heic1611c.tif

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Summary

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 & filters Band	Wavelength	Telescope 
Optical V           	555 nm  	Hubble Space Telescope WFC3
Optical Broad Band	350 nm  	Hubble Space Telescope WFC3
Optical I       	814 nm  	Hubble Space Telescope WFC3
.
Date 2 June 2016, 17:30 (Release)
Source https://www.spacetelescope.org/images/heic1611c/ https://spacetelescope.org/static/archives/images/original/potw1611c.tif
Author Credit: NASA, ESA, and L. Frattare (STScI)
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Date/TimeThumbnailDimensionsUserComment
current21:44, 1 April 2020Thumbnail for version as of 21:44, 1 April 20202,800 × 2,800 (19.71 MB)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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