Fail:Rubin Observatory and Its Target.jpg - Wikipedia Bahasa Melayu, ensiklopedia bebas

Fail asli (7,396 × 4,002 piksel, saiz fail: 8.79 MB, jenis MIME: image/jpeg)

Fail ini dari Wikimedia Commons dan mungkin digunakan oleh projek lain. Penerangan pada laman penerangan failnya di sana ditunjukkan di bawah.

Ringkasan

KeteranganRubin Observatory and Its Target.jpg	English: This image captures not only Vera C. Rubin Observatory, a Program of NSF’s NOIRLab, but one of the celestial specimens Rubin Observatory will observe when it comes online: the Milky Way. The bright halo of gas and stars on the left side of the image highlights the very center of the Milky Way galaxy. The dark path that cuts through this center is known as the Great Rift, because it gives the appearance that the Milky Way has been split in half, right through its center and along its radial arms. In fact, the Great Rift is caused by a shroud of dust, which blocks and scatters visible light. This dust makes the Great Rift a difficult space to observe. Fortunately, Rubin is being built to conduct the Legacy Survey of Space and Time (LSST). This survey will observe the entire visible southern sky every few nights over the course of a decade, capturing about 1000 images of the sky every night and giving us a new view of our evolving Universe. The LSST is set to probe four areas of science, one of which is mapping the Milky Way to answer questions about its structure and formation. Once Rubin Observatory comes online in 2024, scientists will be able to access the data taken every night of operation. Rubin Observatory is a joint initiative of the National Science Foundation and the Department of Energy (DOE). Once completed, Rubin will be operated jointly by NSF’s NOIRLab and DOE's SLAC National Accelerator Laboratory to carry out the Legacy Survey of Space and Time. Español: Esta imagen no sólo captura el Observatorio Vera C. Rubin, un Programa de NOIRLab de NSF, sino que también a uno de los especímenes celestes que el Observatorio Rubin observará cuando entre en funcionamiento: la Vía Láctea. El halo brillante de gas y estrellas en la parte izquierda de la imagen destaca el centro mismo de nuestra galaxia. El sendero oscuro que atraviesa este centro se conoce como la Gran Grieta, porque da la impresión de que la Vía Láctea estuviese partida en dos, justo a través de su centro y a lo largo de sus brazos espirales. En realidad, la Gran Grieta está formada por un manto de polvo que bloquea y dispersa la luz visible, convirtiéndola en un espacio difícil de observar. Por suerte, Rubin se está construyendo para llevar a cabo la Investigación del Espacio-Tiempo como Legado para la Posteridad (LSST por sus siglas en inglés). Esta investigación observará por una década todo el cielo austral visible, capturando unas 1.000 imágenes del cielo cada noche y ofreciéndonos una nueva perspectiva de nuestro Universo en evolución. El LSST está destinado a explorar cuatro áreas de la ciencia, y una de ellas es mapear la Vía Láctea para responder interrogantes sobre su estructura y formación. Una vez que el Observatorio Rubin entre en operación en 2024, los científicos podrán acceder a los datos recopilados en cada noche de operación. El Observatorio Rubin es una iniciativa conjunta de la Fundación Nacional de Ciencias y el Departamento de Energía (DOE). Una vez completado, el Observatorio Rubin será operado conjuntamente por NOIRLab de NSF y el Laboratorio Nacional del Acelerador SLAC de DOE para llevar a cabo el estudio denominado Legacy Survey of Space and Time.
Tarikh	16 Februari 2022, 12:00:00
Sumber	https://noirlab.edu/public/images/iotw2207a/
Pengarang	Rubin Observatory/NSF/AURA/B. Quint

Perlesenan

This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible."
To the uploader: You must provide a link (URL) to the original file and the authorship information if available.

Fail ini dilesenkan di bawah lesen Pengiktirafan 4.0 Antarabangsa Creative Commons.

Anda bebas:

untuk berkongsi – untuk menyalin, mengedar dan memindah hasil kerja
untuk mencampur semula – untuk menyesuaikan karya

Di bawah syarat berikut:

pengiktirafan – Anda mesti memberi penghargaan yang berpatutan, bekalkan pautan ke lesen, dan tunjukkan jika perubahan telah dibuat. Anda boleh lakukannya dalam sebarang cara yang munasabah, tetapi bukan dalam sebarang cara yang mencadangkan pemberi lesen mengendors anda atau penggunaan anda.

Sejarah fail

Klik pada tarikh/waktu untuk melihat rupa fail tersebut pada waktu itu.

	Tarikh/Waktu	Gambar kenit	Ukuran	Pengguna	Komen
semasa	18:00, 22 Jun 2023		7,396 × 4,002 (8.79 MB)	C messier	full size
	19:37, 30 Januari 2023		1,280 × 692 (244 KB)	Yiseth Romero	Uploaded a work by Rubin Observatory/NSF/AURA/B. Quint from https://noirlab.edu/public/images/iotw2207a/ with UploadWizard

Penggunaan fail

35 buah laman berikut menggunakan fail ini:

Penggunaan fail sejagat

Fail ini digunakan oleh wiki-wiki lain yang berikut:

Penggunaan di cs.wikipedia.org
- Vera C. Rubin Observatory
Penggunaan di de.teknopedia.teknokrat.ac.id
- Vera C. Rubin Observatory
Penggunaan di en.wikipedia.org

Lihat banyak lagi penggunaan sejagat bagi fail ini.

Metadata

Fail ini mengandungi maklumat tambahan daripada kamera digital atau pengimbas yang digunakan untuk menghasilkannya. Jika fail ini telah diubah suai daripada rupa asalnya, beberapa butiran dalam maklumat ini mungkin sudah tidak relevan.

Kredit/Pembekal	Rubin Observatory/NSF/AURA/B. Quint
Sumber	NSF's NOIRLab
Tajuk ringkas	Rubin Observatory and Its Target
Tajuk imej	This image captures not only Vera C. Rubin Observatory, a Program of NSF’s NOIRLab, but one of the celestial specimens Rubin Observatory will observe when it comes online: the Milky Way. The bright halo of gas and stars on the left side of the image highlights the very center of the Milky Way galaxy. The dark path that cuts through this center is known as the Great Rift, because it gives the appearance that the Milky Way has been split in half, right through its center and along its radial arms. In fact, the Great Rift is caused by a shroud of dust, which blocks and scatters visible light. This dust makes the Great Rift a difficult space to observe. Fortunately,Rubin is being built to conduct the Legacy Survey of Space and Time (LSST). This survey will observe the entire visible southern sky every few nights over the course of a decade, capturing about 1000 images of the sky every night and giving us a new view of our evolving Universe. The LSST is set toprobe four areas of science, one of which is mapping the Milky Way to answer questions about its structure and formation. Once Rubin Observatory comes online in 2024, scientists will be able to access the data taken every night of operation. Rubin Observatory is a joint initiative of the National Science Foundation and the Department of Energy (DOE). Once completed, Rubin will be operated jointly by NSF’s NOIRLab and DOE's SLAC National Accelerator Laboratory to carry out the Legacy Survey of Space and Time.
Terma-terma penggunaan	Creative Commons Attribution 4.0 International License
Tarikh dan waktu penjanaan data	12:00, 16 Februari 2022
Komen fail JPEG	This image captures not only Vera C. Rubin Observatory, a Program of NSF’s NOIRLab, but one of the celestial specimens Rubin Observatory will observe when it comes online: the Milky Way. The bright halo of gas and stars on the left side of the image highlights the very center of the Milky Way galaxy. The dark path that cuts through this center is known as the Great Rift, because it gives the appearance that the Milky Way has been split in half, right through its center and along its radial arms. In fact, the Great Rift is caused by a shroud of dust, which blocks and scatters visible light. This dust makes the Great Rift a difficult space to observe. Fortunately, Rubin is being built to conduct the Legacy Survey of Space and Time (LSST). This survey will observe the entire visible southern sky every few nights over the course of a decade, capturing about 1000 images of the sky every night and giving us a new view of our evolving Universe. The LSST is set to probe four areas of science, one of which is mapping the Milky Way to answer questions about its structure and formation. Once Rubin Observatory comes online in 2024, scientists will be able to access the data taken every night of operation. Rubin Observatory is a joint initiative of the National Science Foundation and the Department of Energy (DOE). Once completed, Rubin will be operated jointly by NSF’s NOIRLab and DOE's SLAC National Accelerator Laboratory to carry out the Legacy Survey of Space and Time.
Perisian digunakan	Adobe Photoshop 23.0 (Windows)
Tarikh dan waktu fail diubah	10:52, 3 Disember 2021
Tarikh dan waktu pendigitan	04:44, 9 Julai 2021
Tarikh kali terakhir metadata diubah	03:52, 3 Disember 2021
ID unik dokumen asli	xmp.did:63759b61-539f-b945-bab7-92a526b9b8e0
Maklumat hubungan	https://noirlab.edu 950 North Cherry Ave. Tucson, AZ, 85719 USA
Versi IIM	4

Ringkasan

Perlesenan

Captions

Items portrayed in this file

menggambarkan

Vera C. Rubin Observatory ^Inggeris

status hak cipta

berhak cipta

lesen hak cipta

Creative Commons Attribution 4.0 International ^Inggeris

masa permulaan

16 Februari 2022

media type ^Inggeris

image/jpeg

Sejarah fail

Penggunaan fail

Penggunaan fail sejagat

Metadata

Ringkasan

Perlesenan

Captions

Items portrayed in this file

menggambarkan

Vera C. Rubin Observatory Inggeris

status hak cipta

berhak cipta

lesen hak cipta

Creative Commons Attribution 4.0 International Inggeris

masa permulaan

16 Februari 2022

media type Inggeris

image/jpeg

Sejarah fail

Penggunaan fail

Penggunaan fail sejagat

Metadata

Vera C. Rubin Observatory ^Inggeris

Creative Commons Attribution 4.0 International ^Inggeris

media type ^Inggeris