Vaizdas:Birds of a feather (50071190086).jpg
Didesnės raiškos iliustracija (3 913 × 3 345 taškų, rinkmenos dydis: 10,79 MiB, MIME tipas: image/jpeg)
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Aprašymas
AprašymasBirds of a feather (50071190086).jpg |
The spiral pattern shown by the galaxy in this image from the NASA/ESA Hubble Space Telescope is striking because of its delicate, feathery nature. These "flocculent" spiral arms indicate that the recent history of star formation of the galaxy, known as NGC 2775, has been relatively quiet. There is virtually no star formation in the central part of the galaxy, which is dominated by an unusually large and relatively empty galactic bulge, where all the gas was converted into stars long ago. NGC 2275 is classified as a flocculent spiral galaxy, located 67 million light-years away in the constellation of Cancer. Millions of bright, young, blue stars shine in the complex, feather-like spiral arms, interlaced with dark lanes of dust. Complexes of these hot, blue stars are thought to trigger star formation in nearby gas clouds. The overall feather-like spiral patterns of the arms are then formed by shearing of the gas clouds as the galaxy rotates. The spiral nature of flocculents stands in contrast to the grand design spirals, which have prominent, well defined-spiral arms. Credits: ESA/Hubble & NASA, J. Lee and the PHANGS-HST Team; CC BY 4.0
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Data | |
Šaltinis | Birds of a feather |
Autorius | European Space Agency |
Licencija
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This image was originally posted to Flickr by europeanspaceagency at https://flickr.com/photos/37472264@N04/50071190086. It was reviewed on 2020 m. gruodžio 3 d. by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
2020 m. gruodžio 3 d.
Items portrayed in this file
vaizduoja
some value
copyright status anglų
copyrighted anglų
29 birželio 2020
MIME type anglų
image/jpeg
checksum anglų
d6be4971e28678867263d8e31bc431df44f8e129
data size anglų
11 313 854 Baitas
3 345 pikselis
3 913 pikselis
Rinkmenos istorija
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Data/Laikas | Miniatiūra | Matmenys | Naudotojas | Paaiškinimas | |
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dabartinis | 18:03, 3 gruodžio 2020 | 3 913 × 3 345 (10,79 MiB) | Eyes Roger | Transferred from Flickr via #flickr2commons |
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Meta duomenys
Šioje iliustracijoje ar faile yra saugoma papildoma informacija, sukurta skaitmeninio fotoaparato, skenerio. Jei failas yra pakeistas, kai kurios detalės gali ne visai tiksliai aprašyti pakeistą iliustraciją.
Sukūrimo data ir laikas | 06:00, 29 birželio 2020 |
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Trumpas pavadinimas | Birds of a Feather |
Padėka/tiekėjas | ESA/Hubble & NASA, J. Lee and th |
Šaltinis | ESA/Hubble |
Vaizdo pavadinimas | The spiral pattern shown by the galaxy in this image from the NASA/ESA Hubble Space Telescope is striking because of its delicate, feathery nature. These "flocculent" spiral arms indicate that the recent history of star formation of the galaxy, known as NGC 2775, has been relatively quiet. There is virtually no star formation in the central part of the galaxy, which is dominated by an unusually large and relatively empty galactic bulge, where all the gas was converted into stars long ago. NGC 2275 is classified as a flocculent spiral galaxy, located 67 million light-years away in the constellation of Cancer. Millions of bright, young, blue stars shine in the complex, feather-like spiral arms, interlaced with dark lanes of dust. Complexes of these hot, blue stars are thought to trigger star formation in nearby gas clouds. The overall feather-like spiral patterns of the arms are then formed by shearing of the gas clouds as the galaxy rotates. The spiral nature of flocculents stands in contrast to the grand design spirals, which have prominent, well defined-spiral arms. |
Leidėjas | ESA/Hubble |
Naudojimo sąlygos |
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JPEG failas komentarą | The spiral pattern shown by the galaxy in this image from the NASA/ESA Hubble Space Telescope is striking because of its delicate, feathery nature. These "flocculent" spiral arms indicate that the recent history of star formation of the galaxy, known as NGC 2775, has been relatively quiet. There is virtually no star formation in the central part of the galaxy, which is dominated by an unusually large and relatively empty galactic bulge, where all the gas was converted into stars long ago. NGC 2275 is classified as a flocculent spiral galaxy, located 67 million light-years away in the constellation of Cancer. Millions of bright, young, blue stars shine in the complex, feather-like spiral arms, interlaced with dark lanes of dust. Complexes of these hot, blue stars are thought to trigger star formation in nearby gas clouds. The overall feather-like spiral patterns of the arms are then formed by shearing of the gas clouds as the galaxy rotates. The spiral nature of flocculents stands in contrast to the grand design spirals, which have prominent, well defined-spiral arms. |
Pasukimas | Standartinis |
Horizontali raiška | 72 taškai colyje |
Vertikali raiška | 72 taškai colyje |
Naudota programinė įranga | Adobe Photoshop 21.1 (Windows) |
Failas paskutinį kartą keistas | 16:23, 3 kovo 2020 |
Y ir C pozicija | Centruotas |
Exif versija | 2.31 |
Skaitmenizavimo data ir laikas | 20:09, 25 vasario 2020 |
kiekvieno komponento reikšmė |
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Palaikoma Flashpix versija | 1 |
Spalvų pristatymas | sRGB |
IIM versija | 4 |
Raktiniai žodžiai | NGC 2775 |
Bitai komponente |
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Aukštis | 3 345 px |
Plotis | 3 913 px |
Taškų struktūra | RGB |
Komponentų skaičius | 3 |
Kontaktinė informacija |
Karl-Schwarzschild-Strasse 2 Garching bei München, None, D-85748 Germany |
Laikmenos tipas | Observation |
Paskutinį kartą metadata duomenys keisti | 17:23, 3 kovo 2020 |
Unikalus ID orginalus dokumentas | xmp.did:cebdf848-77a1-ff49-a5c9-8337ed8f9fe0 |