NGC 3699
| Planetarischer Nebel NGC 3699 | |
|---|---|
 | |
| Aufnahme des planetarischen Nebels NGC 3699 mittels der ESO Faint Object Spectrograph and Camera montiert am New Technology Telescope. | |
| AladinLite | |
| Sternbild | Zentaur |
| Position Äquinoktium: J2000.0 | |
| Rektaszension | 11h 27m 57,1s [1] |
| Deklination | −59° 57′ 29″[1] |
| Erscheinungsbild | |
| Scheinbare Helligkeit (visuell) | 11,3 mag [2] |
| Scheinbare Helligkeit (B-Band) | 11,0 mag [2] |
| Winkelausdehnung | 2,3′ × 1,7′ [2] |
| Zentralstern | |
| Bezeichnung | HD 306491[3] |
| Scheinbare Helligkeit | 13 mag [4] |
| Spektralklasse | P[4] |
| Physikalische Daten | |
| Rotverschiebung | −0,000053 [3] |
| Radialgeschwindigkeit | −15,8 km/s [3] |
| Entfernung | 4450 ± 499 Lj |
| Durchmesser | 5,4 |
| Alter | 3.000 Jahre |
| Geschichte | |
| Entdeckung | John Herschel |
| Datum der Entdeckung | 1. April 1834 |
| Katalogbezeichnungen | |
| NGC 3699 • PK 292+1.1 • ESO 129-PN21 • GC 2432 • h 3345 • AM 1125-594 | |
NGC 3699 ist ein planetarischer Nebel im Sternbild Zentaur am Südsternhimmel und hat eine Winkelausdehnung von 2,3' und eine scheinbare Helligkeit von 11,0 mag.
Das Objekt wurde am 1. April 1834 von John Herschel entdeckt.[5]
Literatur
- König, Michael & Binnewies, Stefan (2023): Bildatlas der Sternhaufen & Nebel, Stuttgart: Kosmos, S. 227
Weblinks
- astronews.com: Bild des Tages 14. Dezember 2015
- SIMBAD Astronomical Database
Einzelnachweise
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Autor/Urheber: Credit: ESO, Lizenz: CC BY 4.0
A Planetary Nebula Divided
This fetching cloud of gas was imaged by the ESO Faint Object Spectrograph and Camera (EFOSC2) at ESO's La Silla Observatory. It can be found nestled in the busy constellation of Centaurus in the skies of the southern hemisphere.
The cloud of gas — named NGC 3699 — is a planetary nebula. It is distinguished by an irregular mottled appearance and a dark rift, which roughly bisects it.
These objects, despite the name, have nothing to do with planets and are created in the final stages of the evolution of stars similar in mass to the Sun. The name "planetary nebula" arises from the time of their discovery by William Herschel, when they appeared in the telescopes of the time as rounded objects similar in looks to the planets.
Towards the end of their lives, stars like the Sun exhaust the supply of hydrogen in their cores, putting a stop to nuclear reactions. This causes the star's core to contract under the force of gravity and heat up, while the cooler outer layers expand tremendously — the surface of the Sun, for example, will likely engulf the orbit of Earth when it reaches this stage in its evolution. Unusually strong stellar winds push the gaseous outer layers of the star out into space, eventually exposing the core of the star, which begins to emit ultraviolet radiation, ionising the expelled gas, causing the nebula's ethereal glow, and producing beautiful and varied sights, such as the one in this image.
Credit:
ESO
About the Object Name: NGC 3699 Type: • Milky Way : Nebula : Type : Planetary Constellation: Centaurus Coordinates Position (RA): 11 27 58.75 Position (Dec): -59° 57' 11.09" Field of view: 4.45 x 4.45 arcminutes Orientation: North is 1.1° right of vertical
Colours & filters Band Wavelength Telescope Optical Ha 656 nm New Technology Telescope EFOSC Optical R 658 nm New Technology TelescopeEFOSC Optical V 551 nm New Technology Telescope EFOSC Optical B 445 nm New Technology Telescope EFOSC Optical OIII 500 nm New Technology Telescope EFOSC Ultraviolet U 365 nm New Technology Telescope EFOSC.