Dec 2, 2018 · Physical Information: Based on a recessional velocity of 4740 km/sec, NGC 2599 is about 220 million light years away. Given that and its apparent size of 2.8 by 2.5 arcmin, it is about 180 thousand light years across.

NGC 2599 is a Spiral Galaxy in the Cancer constellation. NGC 2599 is situated close to the celestial equator and, as such, it is at least partly visible from both hemispheres in certain times of the year. Given its B magnitude of 13.4, NGC 2599 is visible with the help of a telescope having an aperture of 10 inches (250mm) or more.

NGC 2599 ist eine spiralförmige Radiogalaxie vom Hubble-Typ Sa im Sternbild Krebs auf der Ekliptik. Sie ist schätzungsweise 208 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 180.000 Lichtjahren.

Apr 14, 2020 · The galaxies that exceed 1 \(\sigma \) are indicated in the figure on the right: the triangle is NGC 2599, the square is NGC 753, the cross is NGC 5055, the pentagon is NGC 157, and the asterisk is NGC 4736; the galaxies with the longest rotation curves from the subsample are marked with circles (see Section 2.2).

ngc 2336 - 这是一个大漩涡星系在北极星方向。 ngc 2346 - 这是麒麟座的一个行星状星云。 ngc 2349 - 这是麒麟座的一个疏散星团。 ngc 2359 - 托尔的头盔，这是一个星云; ngc 2360 - 这是大犬座的一个疏散星团。 ngc 2362 - 这是大犬座的一个疏散星团，有时被称为墨西哥跳星。

Media in category "NGC 2599" The following 3 files are in this category, out of 3 total.

The NGC image archive (1st pass) is now complete (23,520 images - 7840 positives, 7840 negatives, 7840 thumbnails - All annotated) - I will be updating the public database with Dr. Corwin's most current puzzle solution files, Steve Gottlieb's visual observations, and finishing up the manual entry of the original NGC catalogue before starting in ...

Feb 6, 2025 · 발광성운인 Gum 31또는 IC 2599에 둘러싸여 있으며 이 성운에서 약 1,200만년전 생겨났다고 추정되는 중이다. 주로 뜨겁고 매우 큰 항성 들로 이루어져 있으며 그중에는 적색초거성 이나 청색초거성 도 포함되어 있다.

Sep 11, 2023 · Physical Information: Based on a recessional velocity of 505 km/sec, NGC 2500 is about 24 million light years away, but for small distances peculiar (non-Hubble expansion) velocities can significantly affect the accuracy of such distance estimates.

NGC 3324 and IC 2599 are jointly referred to as the Gabriela Mistral Nebula, after the Chilean poet. NGC 3324 lies 9,100 light-years away and has a radius of 15 light years. Both NGC 3293 and NGC 3324 are around 12 million light-years old and show a degree of mass segregation. The more massive members of the cluster are concentrated near the ...