Dosya:Hubble NGC6530.jpg

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ŞınasnayışHubble NGC6530.jpg	A portion of the open cluster NGC 6530 appears as a roiling wall of smoke studded with stars in this image from the NASA/ESA Hubble Space Telescope. NGC 6530 is a collection of several thousand stars lying around 4,350 light-years from Earth in the constellation Sagittarius. The cluster is set within the larger Lagoon Nebula, a gigantic interstellar cloud of gas and dust. Hubble has previously imaged the Lagoon Nebula several times, including these images: [1][2] released in 2010 and 2011. It is the nebula that gives this image its distinctly smoky appearance; clouds of interstellar gas and dust stretch from one side of the image to the other.
Tarix	16 Kanun 2022
Çıme	NASA
Nuştekar	ESA/Hubble & NASA, O. De Marco; Acknowledgment: M.H. Özsaraç

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	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: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[3] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [4] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [5] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

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nıkayên	01:39, 25 Kanun 2022		3,880 - 3,845 (4.05 MB)	Liandrei	{{Information \|Description= View of NGC6530 taken by the Hubble Space Telescope. Text credit: European Space Agency (ESA) \|Source= https://www.nasa.gov/image-feature/goddard/2022/hubble-views-a-star-studded-cosmic-cloud NASA \|Date= 2022-12-16 \|Author= ESA/Hubble & NASA, O. De Marco; Acknowledgment: M.H. Özsaraç \|Permission= \|other_versions= }}

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Çıme	ESA/Hubble
Kredi/Destegdaren	ESA/Hubble & NASA, ESO, O. De MarcoAcknowledgement: M. H. Özsaraç
Sernuşteyo qıckek	Cosmic Smokescreen
Image title	A portion of the open cluster NGC 6530 appears as a roiling wall of smoke studded with stars in this image from the NASA/ESA Hubble Space Telescope. NGC 6530 is a collection of several thousand stars lying around 4350 light-years from Earth in the constellation Sagittarius. The cluster is set within the larger Lagoon Nebula, a gigantic interstellar cloud of gas and dust. It is the nebula that gives this image its distinctly smokey appearance; clouds of interstellar gas and dust stretch from one side of this image to the other.Astronomers investigated NGC 6530 using Hubble’s Advanced Camera for Surveys and Wide Field Planetary Camera 2. They scoured the region in the hope of finding new examples of proplyds, a particular class of illuminated protoplanetary discs surrounding newborn stars. The vast majority of proplyds have been found in only one region, the nearbyOrion Nebula. This makes understanding their origin and lifetimes in other astronomical environments challenging.Hubble’s ability to observe at infrared wavelengths — particularly with Wide Field Camera 3— have made it an indispensable tool for understanding starbirth and the origin of exoplanetary systems. In particular, Hubble was crucial to investigations of the proplyds around newly born stars in the Orion Nebula. The new NASA/ESA/CSA James Webb Space Telescope’s unprecedented observational capabilities at infrared wavelengths will complement Hubble observations by allowing astronomers to peer through the dusty envelopes around newly born stars and investigate the faintest, earliest stages of starbirth.[Image description: Clouds of gas cover the entire view, in a variety of bold colours. In the centre the gas is brighter and very textured, resembling dense smoke. Around the edges it is more sparse and faint. Several small, bright blue stars are scattered over the nebula.]
Şertê karkerdışi	Creative Commons Attribution 4.0 International License
Date and time of data generation	06:00, 12 Kanun 2022
Karenaye nusnerek	Adobe Photoshop 24.0 (Windows)
File change date and time	16:33, 9 Kanun 2022
Demê dijitalkerdışi	12:23, 29 Keşkelun 2022
Malumatê metamalumati peyd timarya	17:33, 9 Kanun 2022
Xasiya ID ya dokuman de orcinali	xmp.did:d077763c-ef0d-4c45-ab7a-b2bd0b39d17e
Çekuyên kıliti	Lagoon Nebula NGC 6530
Melumatê irtıbati	https://esahubble.org ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States
Verqaydê IIM	4

Dosya:Hubble NGC6530.jpg

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16 Kanun 2022

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