File:Aldebaran.jpg

File
File history
File usage
Metadata

Size of this preview: 600 × 600 pixels. Other resolutions: 240 × 240 pixels | 480 × 480 pixels | 768 × 768 pixels | 1,024 × 1,024 pixels | 1,500 × 1,500 pixels.

Original file ‎(1,500 × 1,500 pixels, file size: 3.03 MB, MIME type: image/jpeg)

This file is from Wikimedia Commons and may be used by other projects. The description on its file description page there is shown below.

Summary

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

Licensing

This file is licensed under the Creative Commons Attribution-Share Alike 4.0 International license.

You are free:

to share – to copy, distribute and transmit the work
to remix – to adapt the work

Under the following conditions:

attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.

File history

Click on a date/time to view the file as it appeared at that time.

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

File usage

The following page uses this file:

Al De Baran

Metadata

This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.

If the file has been modified from its original state, some details may not fully reflect the modified file.

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.
Date and time of data generation	16:00, 9 May 2013
Horizontal resolution	300 dpi
Vertical resolution	300 dpi
Software used	GIMP 2.10.0
File change date and time	18:48, 29 August 2019
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.
Unique ID of original document	xmp.did:6d6c436e-9413-46a7-a215-e1f35f7c4571
Credit/Provider	NASA, ESA, and STScI.
Source	ESA/Hubble
Keywords	Hyades, WD0421+162, WD0431+126
Short title	Overview of the Hyades star cluster (ground-based image)
Contact information	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany
Usage terms	Creative Commons Attribution 4.0 International License
IIM version	4
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.

Anonymous

Search

File:Aldebaran.jpg

Namespaces

More

Page actions

Summary

Licensing

Captions

Items portrayed in this file

depicts

Aldebaran

copyright status

copyrighted

copyright license

Creative Commons Attribution-ShareAlike 4.0 International

inception

9 May 2013

media type

image/jpeg

checksum

3282827a40c2f8bfefecdbccbb9b0f938f6af4f8

data size

3,179,840 byte

height

1,500 pixel

width

1,500 pixel

File history

File usage

Metadata

Navigation

Navigation

Wiki tools

Wiki tools

Anonymous

Search

File:Aldebaran.jpg

Summary

Licensing

Captions

Items portrayed in this file

9 May 2013

image/jpeg

3282827a40c2f8bfefecdbccbb9b0f938f6af4f8

3,179,840 byte

1,500 pixel

1,500 pixel

File history

File usage

Metadata

Navigation

Wiki tools

Page tools