File:Aldebaran.jpg

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DescriptionAldebaran.jpg	English: Picture of Aldebaran. Cropped from File:Hyades cluster.jpg Français : Image d'Aldébaran. Croppée à partir de File:Hyades cluster.jpg
Date	9 May 2013, 16:00:00
Source	https://www.spacetelescope.org/images/heic1309c/
Author	NASA, ESA, and STScI

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	16:55, 29 August 2019		1,500 × 1,500 (3.03 MB)	Romuald 2	User created page with UploadWizard

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Usage on bn.wikipedia.org
- রোহিণী
Usage on en.wikipedia.org
- User:YLSBeta/Userboxes
Usage on fr.wikipedia.org
- Aldébaran
Usage on ja.wikipedia.org
- アルデバラン
- ハスター
Usage on kk.wikipedia.org
- Альдебаран
Usage on nl.wikipedia.org
- Hemellichaam
Usage on ru.wikipedia.org
- Альдебаран
- Список звёзд в пределах 65—70 световых лет
Usage on ru.wikinews.org
- Категория:Список звёзд в пределах 65—70 световых лет
Usage on sk.wikipedia.org
- Aldebaran
Usage on uz.wikipedia.org
- Aldebaran
Usage on www.wikidata.org
- Q12170

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User comments	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.
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
JPEG 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.
Horizontal resolution	300 dpi
Vertical resolution	300 dpi
Software used	GIMP 2.10.0
File change date and time	18:48, 29 August 2019
Unique ID of original document	xmp.did:6d6c436e-9413-46a7-a215-e1f35f7c4571
Keywords	Hyades, WD0421+162, WD0431+126
Contact information	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany
IIM version	4

File:Aldebaran.jpg

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Aldebaran

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inception

9 May 2013

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image/jpeg

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3,179,840 byte

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1,500 pixel

width

1,500 pixel

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