Sary:The light of knowledge (potw2438a).jpg
Rakitra niaviana (3 666 × 4 236 teboka, haben'ilay rakitra : 5,98 Mio, endrika MIME : image/jpeg)
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VisavisaThe light of knowledge (potw2438a).jpg |
English: The magnificent galaxy featured in this Hubble Picture of the Week is NGC 1559. It is a barred spiral galaxy located in the constellation Reticulum near the Large Magellanic Cloud, but much more distant at approximately 35 million light-years from Earth. Hubble last visited this object in 2018. The brilliant light captured in this image offers a wealth of information, which thanks to Hubble can be put to use by both scientists and the public.This picture is composed of a whopping ten different images taken by the Hubble Space Telescope, each filtered to collect light from a specific wavelength or range of wavelengths. It spans Hubble’s sensitivity to light, from ultraviolet around 275 nanometres through blue, green and red to near-infrared at 1600 nanometres. This allows information about many different astrophysical processes in the galaxy to be recorded: a notable example is the red 656-nanometre filter used here. Hydrogen atoms which get ionised can emit light at this particular wavelength, called H-alpha emission. New stars forming in a molecular cloud, made mostly of hydrogen gas, emit copious amounts of ultraviolet light which is absorbed by the cloud, but which ionises it and causes it to glow with this H-alpha light. Therefore, filtering to detect only this light provides a reliable means to detect areas of star formation (called H II regions), shown in this image by the bright red and pink colours of the blossoming patches filling NGC 1559’s spiral arms.These ten images come from six different observing programmes with Hubble, running from 2009 all the way up to the present year. These programmes were led by teams of astronomers from around the world with a variety of scientific goals, ranging from studying ionised gas and star formation, to following up on a supernova, to tracking variable stars as a contribution to calculating the Hubble constant. The data from all of these observations live on in the Hubble archive, available for anyone to use — not only for new science, but also to create spectacular images like this one! This image of NGC 1559, then, is a reminder of the incredible opportunities that the Hubble Space Telescope has provided and continues to provide.Besides Hubble’s observations, astronomers are using the NASA/ESA/CSA James Webb Space Telescope to research this galaxy in even greater depth. This Webb image from February showcases the galaxy in near- and mid-infrared light.[Image Description: A spiral galaxy, tilted at an angle, with irregularly-shaped arms. It appears large and close-up. The centre glows in a yellowish colour, while the disc around it is a bluer colour, due to light from older and newer stars. Dark reddish threads of dust cover the galaxy, and there are many large, shining pink spots in the disc, where stars are forming.] |
Daty | 16 Septambra 2024 (date de téléversement) |
Loharano | The light of knowledge |
Mpamorona azy | ESA/Hubble & NASA, F. Belfiore, W. Yuan, J. Lee and the PHANGS-HST Team, A. Riess, K. Takáts, D. de Martin & M. Zamani (ESA/Hubble) |
Versiona hafa |
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Navoaka tambanin'ny lisansy
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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télescope spatial Hubble Frantsay
statut des droits d'auteur Frantsay
sous droit d'auteur Frantsay
licence Frantsay
type MIME Frantsay
image/jpeg
hauteur Frantsay
4 236 pixel
largeur Frantsay
3 666 pixel
taille des données Frantsay
6 269 697 octet
pris avec Frantsay
Wide Field Camera 3 Frantsay
somme de contrôle Frantsay
002eb3b6fe5878d5dc4e9a94453294b1e2aaa356
16 Septambra 2024
source du fichier Frantsay
somme de contrôle pHash Frantsay
bmcuo4u84zixqctsf39matyjdd2zmr6puf6htu1tlljd86pkz
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Daty sy ora | saritapaka | Habe | Mpikambana | resaka | |
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ankehitriny | 16 Septambra 2024 à 09:01 | 3 666 × 4 236 (5,98 Mio) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esahubble.org/archives/images/large/potw2438a.jpg via Commons:Spacemedia |
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Metadata
Mirakitra fampahalalana fanampiny, izay inoana ho napetraky ny fakan-tsary na scanner nampiasaina nanaovana ny numérisation-ny ity rakitra ity. Raha kitihina na ovana izy ity dia mety tsy hifanitsy amin'ny sary voaova ireo antsipirihany sasany ireo.
Fiaviana | ESA/Hubble |
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Isaorana/mpanome | ESA/Hubble & NASA, F. Belfiore, W. Yuan, J. Lee and the PHANGS-HST Team, A. Riess, K. Takáts, D. de Martin & M. Zamani (ESA/Hubble) |
Fepe-pampiasana |
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Lohateny fohy |
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Visavisan'ilay sary |
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Daty fangalana niaviana | 16 Septambra 2024 à 06:00 |
Resa-drakitra JPEG | The magnificent galaxy featured in this Hubble Picture of the Week is NGC 1559. It is a barred spiral galaxy located in the constellation Reticulum near the Large Magellanic Cloud, but much more distant at approximately 35 million light-years from Earth. Hubble last visited this object in 2018. The brilliant light captured in this image offers a wealth of information, which thanks to Hubble can be put to use by both scientists and the public. This picture is composed of a whopping ten different images taken by the Hubble Space Telescope, each filtered to collect light from a specific wavelength or range of wavelengths. It spans Hubble’s sensitivity to light, from ultraviolet around 275 nanometres through blue, green and red to near-infrared at 1600 nanometres. This allows information about many different astrophysical processes in the galaxy to be recorded: a notable example is the red 656-nanometre filter used here. Hydrogen atoms which get ionised can emit light at this particular wavelength, called H-alpha emission. New stars forming in a molecular cloud, made mostly of hydrogen gas, emit copious amounts of ultraviolet light which is absorbed by the cloud, but which ionises it and causes it to glow with this H-alpha light. Therefore, filtering to detect only this light provides a reliable means to detect areas of star formation (called H II regions), shown in this image by the bright red and pink colours of the blossoming patches filling NGC 1559’s spiral arms. These ten images come from six different observing programmes with Hubble, running from 2009 all the way up to the present year. These programmes were led by teams of astronomers from around the world with a variety of scientific goals, ranging from studying ionised gas and star formation, to following up on a supernova, to tracking variable stars as a contribution to calculating the Hubble constant. The data from all of these observations live on in the Hubble archive, available for anyone to use — not only for new science, but also to create spectacular images like this one! This image of NGC 1559, then, is a reminder of the incredible opportunities that the Hubble Space Telescope has provided and continues to provide. Besides Hubble’s observations, astronomers are using the NASA/ESA/CSA James Webb Space Telescope to research this galaxy in even greater depth. This Webb image from February showcases the galaxy in near- and mid-infrared light. [Image Description: A spiral galaxy, tilted at an angle, with irregularly-shaped arms. It appears large and close-up. The centre glows in a yellowish colour, while the disc around it is a bluer colour, due to light from older and newer stars. Dark reddish threads of dust cover the galaxy, and there are many large, shining pink spots in the disc, where stars are forming.] |
Fampahalalana mikasika ny fifandraisana |
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr 21218 Baltimore, MD United States |
Tenifototra | NGC 1559 |
filaza IIM | 4 |