Fayl:Aldebaran.jpg

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Asl fayl ‎(1 500 × 1 500 piksel, fayl hajmi: 3,03 MB, MIME tipi: image/jpeg)

Ushbu fayl Vikiomborga yuklangan boʻlib, boshqa loyihalarda ham qoʻllanilishi mumkin. Uning tavsif sahifasidan olingan maʼlumot quyida keltirilgan.

Qisqa izoh

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

Litsenziyalash

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

Siz erkinsiz:

ulashishga – ishlanmani nusxalash, tarqatish va uzatish
remiks qilishga – ishni moslashtirishga

Quyidagi shartlar asosida:

atribut – Siz tegishli litsenziyaga havolani taqdim etishingiz va oʻzgartirishlar kiritilganligini koʻrsatishingiz kerak. Siz buni har qanday oqilona yoʻl bilan qilishingiz mumkin, lekin litsenziar Sizni yoki Sizning foydalanishingizni ma'qullashini taklif qiladigan tarzda emas.
bir xil ulashish – Agar Siz materialni remiks qilsangiz, oʻzgartirsangiz yoki unga asoslansangiz, oʻz hissalaringizni asl nusxadagi kabi bir xil yoki mos litsenziya ostida tarqatishingiz kerak.

Fayl tarixi

Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.

	Sana/Vaqt	Miniatura	Oʻlchamlari	Foydalanuvchi	Izoh
joriy	16:55, 29-Avgust 2019		1 500 × 1 500 (3,03 MB)	Romuald 2	User created page with UploadWizard

Fayllarga ishoratlar

Bu faylga quyidagi sahifa bogʻlangan:

Aldebaran

Faylning global foydalanilishi

Ushbu fayl quyidagi vikilarda ishlatilyapti:

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

Metama’lumot

Bu fayl qoʻshimcha maʼlumotlarni oʻz ichiga oladi, ehtimol uni tuzish yoxud raqamlashtirish uchun raqamli kamera yoki skanerdan foydalanilgan.

Agar fayl asl holatidan oʻzgartirilgan boʻlsa, baʼzi tafsilotlar oʻzgartirilgan faylni toʻliq aks ettirmasligi mumkin.

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-Avgust 2019
Unique ID of original document	xmp.did:6d6c436e-9413-46a7-a215-e1f35f7c4571
Keywords	Hyades, WD0421+162, WD0431+126
Contact information	-{R\|http://www.spacetelescope.org/}- Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany
IIM version	4

Fayl:Aldebaran.jpg

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Litsenziyalash

Captions

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tasvirlangan ob'ekt

Aldebaran

mualliflik huquqi holati

mualliflik huquqi himoyalangan

mualliflik huquqi litsenziyasi

Creative Commons Attribution-ShareAlike (xuddi shu shartlar) 4.0 Xalqaro

tashkil etilgan

9 May 2013

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Faylning global foydalanilishi

Metama’lumot

Qisqa izoh

Litsenziyalash

Captions

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9 May 2013

image/jpeg

checksum inglizcha

3282827a40c2f8bfefecdbccbb9b0f938f6af4f8

data size inglizcha

3 179 840 Bayt

1 500 piksel

width inglizcha

1 500 piksel

Fayl tarixi

Fayllarga ishoratlar

Faylning global foydalanilishi

Metama’lumot

checksum ^inglizcha

data size ^inglizcha

width ^inglizcha