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В центре туманности Лагуна APOD: 2023 June 19 Б The Busy Center of the Lagoon Nebula
19.06.2023

The center of the Lagoon Nebula is a whirlwind of spectacular star formation. Visible near the image center, at least two long funnel-shaped clouds, each roughly half a light-year long, have been formed by extreme stellar winds and intense energetic starlight. A tremendously bright nearby star, Herschel 36, lights the area.



Лицом к NGC 6946 Facing NGC 6946
26.07.2024

From our vantage point in the Milky Way Galaxy, we see NGC 6946 face-on. The big, beautiful spiral galaxy is located just 20 million light-years away, behind a veil of foreground dust and stars in the high and far-off constellation Cepheus.



IC 5146: туманность Кокон APOD: 2024 August 19 Б IC 5146: The Cocoon Nebula
19.08.2024

Inside the Cocoon Nebula is a newly developing cluster of stars. Cataloged as IC 5146, the beautiful nebula is nearly 15 light-years wide. Soaring high in northern summer night skies, it's located some 4,000 light years away toward the constellation of the Swan (Cygnus).



M41: звездное скопление Малый Улей APOD: 2025 February 25 Б M41: The Little Beehive Star Cluster
25.02.2025

Why are there so many bright blue stars? Stars are usually born in clusters, and the brightest and most massive of these stars typically glow blue. Less-bright, non-blue stars like our Sun surely also exist in this M41 star cluster but are harder to see. A few bright orange-appearing red giant stars are visible.



NGC 2170: туманность Ангел APOD: 2026 May 19 Б NGC 2170: The Angel Nebula
19.05.2026

Is this a painting or a photograph? In this celestial abstract art composed with a cosmic brush, dusty nebula NGC 2170, also known as the Angel Nebula, shines just above the image center. Reflecting...



M27: туманность Гантель M27: The Dumbbell Nebula
6.03.2001

The first hint of what will become of our Sun was discovered inadvertently in 1764. At that time, Charles Messier was compiling a list of "annoying" diffuse objects not to be confused with "interesting" comets.



Тихо и Коперник: лунные кратеры с лучами Tycho and Copernicus: Lunar Ray Craters
9.08.2001

Dazzling in binoculars or a small telescope, the Moon is pocked with impact craters. During partial lunar phases, the craters along the terminator are cast in dramatic relief by strong shadows. But when the Moon is full some craters seem to sprout systems of bright radial lines or rays.



В центре M15 At the Core of M15
20.11.1995

Densely packed stars in the core of the globular cluster M15 are shown in this Hubble Space Telescope (HST) image taken in April of 1994. The stars revealed are contained in an area 1.6 light years across and their colors roughly indicate their temperatures - hot stars appear blue, cooler stars look reddish-orange.



Туманность Ориона в линиях кислорода, водорода и серы Orion Nebula in Oxygen, Hydrogen, and Sulfur
13.07.2004

The Great Nebula in Orion, an immense, nearby starbirth region, is arguably the most famous of all astronomical nebulae. The Orion Nebula, also known as M42, is shown above through ultraviolet and blue filters augmented with three exact colors specifically emitted by hydrogen, oxygen, and sulfur.



M2-9: крылья туманности Бабочка M2 9: Wings of a Butterfly Nebula
27.12.1998

Are stars better appreciated for their art after they die? Actually, stars usually create their most artistic displays as they die. In the case of low-mass stars like our Sun and M2-9 pictured above, the stars transform themselves from normal stars to white dwarfs by casting off their outer gaseous envelopes.




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