NGC 4694
| Galaxie NGC 4694 | |
|---|---|
 | |
| Aufnahme der Galaxie mithilfe des Hubble-Weltraumteleskops | |
| AladinLite | |
| Sternbild | Jungfrau |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 12h 48m 15,1s[1] |
| Deklination | +10° 59′ 01″[1] |
| Erscheinungsbild | |
| Morphologischer Typ | SB0 / HII[1][2] |
| Helligkeit (visuell) | 11,1 mag[2] |
| Helligkeit (B-Band) | 12,1 mag[2] |
| Winkelausdehnung | 3,3′ × 1,6′[2] |
| Positionswinkel | 140°[2] |
| Flächenhelligkeit | 12,8 mag/arcmin²[2] |
| Physikalische Daten | |
| Zugehörigkeit | Virgo-Cluster Messier 49-Gruppe NGC 4636-Gruppe NGC 4343-Gruppe LGG 292[1][3] |
| Rotverschiebung | 0,003869 ± 0,000008[1] |
| Radialgeschwindigkeit | (1160 ± 2) km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) | (50 ± 4) · 106 Lj (15,2 ± 1,1) Mpc [1][2] |
| Geschichte | |
| Entdeckung | Wilhelm Herschel |
| Entdeckungsdatum | 15. März 1784 |
| Katalogbezeichnungen | |
| NGC 4694 • UGC 7969 • PGC 43241 • CGCG 071-044 • MCG +02-33-023 • IRAS 12457+1115 • 2MASX J12481509+1059010 • VCC 2066 • GC 3225 • H II 72 • h 1434 • HIPASS J1247+10 • LDCE 904 NED250 • EVCC 1171 | |
NGC 4694 ist eine Linsenförmige Galaxie mit ausgedehnten Sternentstehungsgebieten vom Hubble-Typ SB0 im Sternbild Jungfrau auf der Ekliptik. Sie ist schätzungsweise 50 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 50.000 Lichtjahren. Unter der Katalognummer VCC 2066 ist sie als Mitglied des Virgo-Galaxienhaufens aufgeführt. Im selben Himmelsareal befinden sich u. a. die Galaxien NGC 4733, IC 3727, IC 3773, IC 3775.
Das Objekt wurde am 15. März 1784 von dem Astronomen Wilhelm Herschel mithilfe seines 18,7 Zoll-Spiegelteleskops entdeckt.[4]
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Most galaxies we are familiar with fall into one of two easily-identified types. Spiral galaxies are young and energetic, filled with the gas needed to form new stars and sporting spiral arms hosting hot, bright stars. Elliptical galaxies have a much more pedestrian look, their light coming from a uniform population of older and redder stars. But other galaxies require in-depth study to understand: such is the case with NGC 4694, a galaxy located 54 million light-years from Earth in the Virgo galaxy cluster, and the subject of this Hubble Picture of the Week.
NGC 4694 has a smooth-looking, armless disc which— like an elliptical galaxy — is nearly devoid of star formation. However its stellar population is still relatively young and new stars are still actively forming in its core, powering the brightness we can see in this image and giving it a markedly different stellar profile from that of a classic elliptical galaxy. The galaxy is also suffused by the kinds of gas and dust normally seen in a young and sprightly spiral; elliptical galaxies often do host significant quantities of dust, but not the gas needed to form new stars. NGC 4694 is surrounded by a huge cloud of invisible hydrogen gas,fuel for star formation. This stellar activity is the reason for Hubble’s observations here.
As this Hubble image shows, the dust in this galaxy forms chaotic structures that indicate some kind of disturbance. It turns out that the cloud of hydrogen gas around NGC 4694 forms a long bridge to a nearby, faint dwarf galaxy named VCC 2062. The two galaxies have undergone a violent collision, and the larger NGC 4694 is accreting gas from the smaller galaxy. Based on its peculiar shape and its star-forming activity, NGC 4694 has been classified as a lenticular galaxy: lacking the unmistakable arms of a spiral, but not so bereft of gas as an elliptical galaxy, and still with a galactic bulge and disc. Some galaxies just aren’t so easy to classify as one type or the other!
[Image Description: An oval-shaped galaxy seen tilted at an angle. It glows brightly at its central point, with the radiated light dimming out to the edge of the oval. Reddish-brown, patchy dust spreads out from the core and covers much of the galaxy’s top half, as well as the outer edge, obscuring some of its light. Stars can be seen around and in front of the galaxy.]