NGC 330
| Kugelsternhaufen NGC 330 | |
|---|---|
 | |
| Aufnahme des Hubble-Weltraumteleskops | |
| AladinLite | |
| Sternbild | Tukan |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 00h 56m 17,6s [1] |
| Deklination | −72° 27′ 47″ [1] |
| Erscheinungsbild | |
| Helligkeit (visuell) | +9,55 mag [2] |
| Helligkeit (B-Band) | +9,76 mag [2] |
| Winkelausdehnung | 1,4' [3] |
| Farbexzess E(B-V) (Rötung) | 0,037 [1] |
| Physikalische Daten | |
| Zugehörigkeit | Kleine Magellansche Wolke |
| Geschichte | |
| Entdeckung | James Dunlop |
| Entdeckungsdatum | 1. August 1826 |
| Katalogbezeichnungen | |
| NGC 330 • ESO 29-SC24 • Dun 23 • GC 183 • Lindsay 54 • Kron 35 • h 2367 | |
NGC 330 ist ein Kugelsternhaufen in der Kleinen Magellanschen Wolke im Sternbild Tukan. NGC 330 hat einen Durchmesser von 1,4' und eine scheinbare Helligkeit von 9,6 mag. Der Kugelsternhaufen zählt aufgrund seines geringen Alters zu der Klasse der jungen blauen Kugelsternhaufen.
Der Kugelsternhaufen NGC 330 wurde am 1. August 1826 von dem schottischen Astronomen James Dunlop entdeckt.[4]
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Credit:
ESA/Hubble & NASA, J. Kalirai, A. Milone, Lizenz: CC BY 4.0A Scattering of Stars
This Picture of the Week depicts the open star cluster NGC 330, which lies around 180,000 light-years away inside the Small Magellanic Cloud. The cluster — which is in the constellation Tucana (The Toucan) — contains a multitude of stars, many of which are scattered across this striking image.
Pictures of the Week from the NASA/ESA Hubble Space Telescope show us something new about the Universe. This image, however, also contains clues about the inner workings of Hubble itself. The criss-cross patterns surrounding the stars in this image — known as diffraction spikes — were created when starlight interacted with the four thin vanes supporting Hubble’s secondary mirror.
As star clusters form from a single primordial cloud of gas and dust, all the stars they contain are roughly the same age. This makes them useful natural laboratories for astronomers to learn how stars form and evolve. This image uses observations from Hubble’s Wide Field Camera 3, and incorporates data from two very different astronomical investigations. The first aimed to understand why stars in star clusters appear to evolve differently from stars elsewhere, a peculiarity first observed by the Hubble Space Telescope. The second aimed to determine how large stars can be before they become doomed to end their lives in cataclysmic supernova explosions.
Credit:
ESA/Hubble & NASA, J. Kalirai, A. Milone
Coordinates Position (RA): 0 56 19.74 Position (Dec): -72° 27' 58.39" Field of view: 2.55 x 2.43 arcminutes Orientation: North is 28.3° left of vertical Colours & filters Band Wavelength Telescope Ultraviolet UV 225 nm Hubble Space Telescope WFC3 Optical U 336 nm Hubble Space Telescope WFC3 Optical U 336 nm Hubble Space Telescope WFC3 Optical I 814 nm Hubble Space Telescope WFC3 Optical H-alpha 656 nm Hubble Space Telescope WFC3 Optical I 814 nm Hubble Space Telescope WFC3.