اصل فائل(۱,۵۹۰ × ۱,۵۹۰ پکسلز, فائل حجم: ۲۴۹ کلوبائٹ, MIME type: image/jpeg)

ایہ فائل Wikimedia Commons توں اے تے دوجیاں ویونتاں تے وی ورتی جاسکدی اے۔ گل بات اس دے فائل گل بات صفحہ تے تھلے دتی گئی۔

خلاصہ

تفصیل

The Boomerang Nebula is a young planetary nebula and the coldest object found in the Universe so far. The NASA/ESA Hubble Space Telescope image is yet another example of how Hubble's sharp eye reveals surprising details in celestial objects.

This NASA/ESA Hubble Space Telescope image shows a young planetary nebula known (rather curiously) as the Boomerang Nebula. It is in the constellation of Centaurus, 5000 light-years from Earth. Planetary nebulae form around a bright, central star when it expels gas in the last stages of its life.

The Boomerang Nebula is one of the Universe's peculiar places. In 1995, using the 15-metre Swedish ESO Submillimetre Telescope in Chile, astronomers Sahai and Nyman revealed that it is the coldest place in the Universe found so far. With a temperature of -272C, it is only 1 degree warmer than absolute zero (the lowest limit for all temperatures). Even the -270C background glow from the Big Bang is warmer than this nebula. It is the only object found so far that has a temperature lower than the background radiation.

Keith Taylor and Mike Scarrott called it the Boomerang Nebula in 1980 after observing it with a large ground-based telescope in Australia. Unable to see the detail that only Hubble can reveal, the astronomers saw merely a slight asymmetry in the nebula's lobes suggesting a curved shape like a boomerang. The high-resolution Hubble images indicate that 'the Bow tie Nebula' would perhaps have been a better name.

The Hubble telescope took this image in 1998. It shows faint arcs and ghostly filaments embedded within the diffuse gas of the nebula's smooth 'bow tie' lobes. The diffuse bow-tie shape of this nebula makes it quite different from other observed planetary nebulae, which normally have lobes that look more like 'bubbles' blown in the gas. However, the Boomerang Nebula is so young that it may not have had time to develop these structures. Why planetary nebulae have so many different shapes is still a mystery.

The general bow-tie shape of the Boomerang appears to have been created by a very fierce 500 000 kilometre-per-hour wind blowing ultracold gas away from the dying central star. The star has been losing as much as one-thousandth of a solar mass of material per year for 1500 years. This is 10-100 times more than in other similar objects. The rapid expansion of the nebula has enabled it to become the coldest known region in the Universe.

The image was exposed for 1000 seconds through a green-yellow filter. The light in the image comes from starlight from the central star reflected by dust particles.
تریخ
سروت http://www.spacetelescope.org/images/heic0301a/
لکھاری ESA/NASA
اجازت
(فائل نوں دوبارہ ورتنا)
Public domain This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.
For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

لائسنس –

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

چترن

۲۰ فروری 2003

media type English

image/jpeg

checksum English

42c243802b26913bf892b86072843cbf5f84b05f

determination method English: ؜SHA-1 English

data size English

۲۵۵,۲۱۲ بائٹ

height English

۱,۵۹۰ pixel

width English

۱,۵۹۰ pixel

فائل دی تریخ

فائل نو اس ویلے دی حالت وچ ویکھن واسطے تاریخ/ویلے تے کلک کرو۔

تریخ تے ویلہنکی مورتپاسےورتن والاتیپّݨی کرو
موجودہ۲۰:۲۹, ۱۹ مئی ۲۰۰۷۲۰:۲۹, ۱۹ مئی ۲۰۰۷ ویلے دے ورژن ساتھ انگوٹھاکار روپ۱,۵۹۰ × ۱,۵۹۰ (۲۴۹ کلوبائٹ)Pamputt{{Information |Description= |Source= |Date= |Author= |Permission= |other_versions= }}

تھلے دتے گئے 1 صفحے اس فائل نال جُڑدے نیں

فائل ویاپک ورتوں

ایہہ دوجے وکیاں ایس فائل نوں ورتدے نیں –

ایس فائل دا ویکھو ہور جگت ورتن .

میٹا ڈیٹا