File:HD28527 Location.png

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The location of HD 28527 within the Hyades star cluster

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DescriptionHD28527 Location.png	English: The location of HD 28527 within the Hyades star cluster
Date	2 September 2022
Source	https://upload.wikimedia.org/wikipedia/commons/b/b0/Hyades_cluster.jpg
Author	Unknown, I modified a file from Wikipedia Commons by adding an arrow to point to the star HD 28527

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	12:32, 2 September 2022		6,334 × 4,937 (41.99 MB)	PopePompus (talk \| contribs)	Uploaded a work by Unknown, I modified a file from Wikipedia Commons by adding an arrow to point to the star HD 28527 from https://upload.wikimedia.org/wikipedia/commons/b/b0/Hyades_cluster.jpg with UploadWizard

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Credit/Provider	NASA, ESA, and STScI.
Source	ESA/Hubble
Image title	This image shows the Hyades star cluster, the nearest cluster to us. The Hyades cluster is very well studied due to its location, but previous searches for planets have produced only one. A new study led by Jay Farihi of the University of Cambridge, UK, has now found the atmospheres of two burnt-out stars in this cluster— known as white dwarfs — to be “polluted” by rocky debris circling the star. Seeing evidence of asteroids points to the possibility of Earth-sized planets in the same system, as asteroids are the building blocks of major planets. Planet-forming processes are inefficient, and spawn many times more small bodies than large bodies — but once rocky embryos the size of asteroids are built, planets are sure to follow.
Short title	Overview of the Hyades star cluster (ground-based image)
Usage terms	Creative Commons Attribution 4.0 International License
Date and time of data generation	16:00, 9 May 2013
PNG file comment	This image shows the Hyades star cluster, the nearest cluster to us. The Hyades cluster is very well studied due to its location, but previous searches for planets have produced only one. A new study led by Jay Farihi of the University of Cambridge, UK, has now found the atmospheres of two burnt-out stars in this cluster — known as white dwarfs — to be “polluted” by rocky debris circling the star. Seeing evidence of asteroids points to the possibility of Earth-sized planets in the same system, as asteroids are the building blocks of major planets. Planet-forming processes are inefficient, and spawn many times more small bodies than large bodies — but once rocky embryos the size of asteroids are built, planets are sure to follow.
Unique ID of original document	xmp.did:7b103d35-258a-4756-a0d2-7bc7e6777fc9
Software used	GIMP 2.10
Keywords	Hyades WD0421+162 WD0431+126
Contact information	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany
Horizontal resolution	118.11 dpc
Vertical resolution	118.11 dpc
File change date and time	12:19, 2 September 2022

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