NGC 3274 - HST - Potw1647a

(c) ESA/Hubble, CC BY 4.0

Autor/Urheber:
ESA/Hubble & NASA, D. Calzetti
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Hubble spies NGC 3274

This image of the spiral galaxy NGC 3274 comes courtesy of the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 (WFC3). Hubble’s WFC3 vision spreads from the ultraviolet light through to the near infrared , allowing astronomers to study a wide range of targets, from nearby star formation through to galaxies in the most remote regions of the cosmos.

This particular image combines observations gathered in five different filters, bringing together ultraviolet, visible, and infrared light to show off NGC 3274 in all its glory. As with all of the data Hubble sends back to Earth, it takes advantage of the telescope’s location in space above our planet’s distorting atmosphere. WFC3 returns clear, crisp, and detailed images time after time.

NGC 3274 is a relatively faint galaxy located over 20 million light-years away in the constellation of Leo (The Lion). The galaxy was discovered by Wilhelm Herschel in 1783. The galaxy PGC 213714 is also visible on the upper right of the frame, located much further away from Earth.

Credit: ESA/Hubble & NASA, D. Calzetti 

Coordinates
Coordinates
Position (RA):	10 32 17.16
Position (Dec):	27° 40' 7.94"
Field of view:	2.64 x 2.30 arcminutes
Orientation:	North is 10.6° left of vertical

Colours & filters
Band	Wavelength	Telescope
Ultraviolet UV	275 nm	Hubble Space Telescope WFC3
Optical U	336 nm	Hubble Space Telescope WFC3
Optical B	438 nm	Hubble Space Telescope WFC3
Optical V	555 nm	Hubble Space Telescope WFC3
Optical I	814 nm	Hubble Space Telescope WFC3
.
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Weitere Informationen zur Lizenz des Bildes finden Sie hier. Letzte Aktualisierung: Wed, 27 Mar 2024 23:56:01 GMT


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NGC 3274

NGC 3274 ist eine balkenspiralförmige Zwerggalaxie vom Hubble-Typ SBcd im Sternbild Löwe an der Ekliptik, die schätzungsweise 22 Millionen Lichtjahre von der Milchstraße entfernt ist. Sie bildet mit der wesentlich weiter entfernten Galaxie PGC 213714 ein optisches Paar. Die Entfernungsmessungen basierend auf den Radialgeschwindigkeiten stimmen nicht mit den rotverschiebungsunabhängigen Entfernungsschätzungen von 41 ± 21 Millionen Lichtjahren überein. .. weiterlesen