NGC 7205 is a spiral galaxy in the constellation Indus. The galaxy lies about 60 million light years away from Earth based on redshift independent methods, which means, given its apparent dimensions, that NGC 7205 is approximately 70,000 light years across. [1] It was discovered by John Herschel on June 10, 1834. [3]

NGC 7205 is a Spiral Galaxy in the Tucana constellation. NGC 7205 is situated south of the celestial equator and, as such, it is more easily visible from the southern hemisphere. Given its B magnitude of 11.77, NGC 7205 is visible with the help of a telescope having an aperture of 8 inches (200mm) or more.

NGC 7205 is a Spiral Galaxy located in the constellation of Tucana in the southern hemisphere. NGC 7205's distance from Earth is 62,390,453.49 light years. NGC 7205 is called NGC 7205 in the New General Catalogue (NGC).

2024年10月5日 · NGC 7205 is a barred spiral galaxy located 71 million light years away in the constellation of Tucana. The arms appear somewhat flocculent and there are prominent dust lanes as well as hydrogen alpha regions.

Physical Information: Based on a recessional velocity relative to the Cosmic Microwave Background radiation of 1535 km/sec (and H0 = 70 km/sec/Mpc), NGC 7205 is about 70 to 75 million light-years away, in good agreement with redshift-independent distance estimates of about 45 to 75 million light-years.

2024年3月19日 · The SIMBAD astronomical database provides basic data, cross-identifications, bibliography and measurements for astronomical objects outside the solar system.

Radial Profiles • summary from 1-D atlas • surface brightness and color profile plot • geometric and Fourier parameters plot • surface brightness ( B, V, R, I) • ellipticity ( B, V, R, I) • position angle ( B, V, R, I)

NGC 7205 58 minutes exposure, Fuji Provia 400 slide film. 5" f/5 refractor, prime focus. Like its neighbouring constellation Grus, the southern constellation of Tucana is rich with faint galaxies that are interesting to hunt down with the telescope.

NGC 7205 este o galaxie situată în constelația Tucanul. [4][5][6] A fost descoperită în 10 iulie 1834 de către John Herschel. [7] Se află la o distanță de 18,97 megaparseci de Pământ.

A similarly broad-line width and largechange in velocity has been noted for the maser in NGC 1052, wherein jetactivity excites the emission. Neither optical spectroscopy,radio-infrared correlations, nor infrared colors provide compellingevidence of unusual activity in the nucleus of IRAS F01063-8034.