NGC 1300 – Spiral galaxy in Eridanus is classified as a spiral galaxy (SAbc) according to the morphological classification of Hubble and de Vaucouleurs. ngc 1300 – Spiral galaxy in Eridanus is classified as a spiral galaxy (SAbc) according to the morphological classification of Hubble and de Vaucouleurs. The lower the number, the brighter the object can be seen. NGC 1300 – Spiral Galaxy in Eridanus is classified as a spiral galaxy (SAbc) according to the morphological classification of Hubble and de Vaucouleurs.
NGC 1300 is not known to have an active core, suggesting that its central black hole does not accrete matter. This is the spiral bar galaxy NGC 1300, which lies 69 million light years from Earth in the constellation Eridanus and has a diameter of about 88,000 light years. Starlight and dust can be seen in blue, visible and infrared light.
What is the name of NGC 1300?
This Hubble Space Telescope image of the beautiful island universe is one of the largest Hubble images ever taken of an entire galaxy. The Hubble telescope captured a spectacle of starlight, glowing gas and dark clouds of interstellar dust in this 1.5 metre by 1.5 metre image of the barred spiral galaxy NGC 1300. NGC 1300, taken with the Hubble Space Telescope Observational data Constellation Eridanus Right ascension 03h 19m 41.1s Declination -19° 24′ 41″ Redshift 0.005260 Distance 61.3 million light years Apparent magnitude (V) 11.4 Properties Type SB(rs), bc Apparent magnitude (V) 6′.
How old is NGC 1300?
This true-colour image was created from fifteen images taken on the night of 24 December 2000 (yes, Christmas Eve) with the Kitt Peak National Observatory’s 2.1-metre telescope in the BVR passbands. At the core of the larger spiral structure of NGC 1300, the nucleus shows its own unusual and distinct spiral structure about 3,300 light-years (1 kiloparsec) long. This true colour image was created from fifteen images taken on the night of December 24, 2000 (yes, Christmas Eve) with the Kitt Peak National Observatory’s 2.1 metre telescope in the BVR pass bands. NGC 1300 is a spiral galaxy with a bar of stars and gas at its centre, located about 61 million light years from Earth in the constellation Eridanus. Only galaxies with large bars seem to have these large-scale inner disks – a spiral within a spiral.
How does NGC 1300 differ from a normal spiral galaxy?
Barred spirals differ from normal spiral galaxies in that the arms of the galaxy do not spiral to the centre, but are connected to the two ends of a straight bar of stars containing the nucleus at the centre. Due to the size of the galaxy, two adjacent alignments of the telescope were required to detect the extent of the spiral arms. This comparison shows two images of NGC 1300, a spiral galaxy with a bar of stars and gas at its centre, located about 61 million light years from Earth in the constellation Eridanus, taken at many different wavelengths of light.
What kind of galaxy is NGC 1313?
This is a NASA Hubble Space Telescope image of the central region of the barred spiral galaxy NGC 1313. The mutual attraction between the galaxies causes immense turbulence in gas and dust, which causes the sudden “burst” of star formation. This is an image taken by NASA’s Hubble Space Telescope of the central region of the barred spiral galaxy NGC 1313: The mutual attraction between the galaxies causes immense turmoil in gas and dust, causing the sudden “burst” of star formation. The spiral arms are a hotbed of star formation, with numerous young clusters of hot stars being born continuously and at dizzying speed from the dense clouds of gas and dust. The clouds of bluish stars appear to have formed randomly, without the usual trigger of gravitational interaction or even pronounced spiral processes to produce them.
The Topsy-Turvy Galaxy (NGC 131) is an unusual spiral starburst galaxy with an extent of about 50,000 light-years, located about 1500 light-years away in the constellation Reticulum.
