Messier 90 (M90): An Intermediate Spiral Galaxy in Virgo

M90, also known as NGC 4548, is a intermediate spiral galaxy located about 60 million light-years away in the Virgo Constellation. This galaxy is a member of the Virgo Cluster of galaxies, a dense region of space containing thousands of galaxies. M90 stands out for its large size, approximately 120,000 light-years in diameter, and its distinctive orientation, which makes it appear almost edge-on from Earth.

M90 is an intermediate spiral galaxy, which places it between a normal spiral galaxy and a barred spiral galaxy. It has a weak or intermediate bar structure with loosely wound spiral arms and moderate star formation activity.

One of the intriguing aspects of M90 is its close interaction with nearby galaxies, particularly IC 3583. IC 3583 is a smaller galaxy that lies just a few million light-years from M90. The two galaxies are in the process of interacting gravitationally, which is significant because their close proximity suggests that they could be exchanging gas, triggering star formation, or even on a collision course that could eventually result in a merger. This interaction is typical in galaxy clusters, where galaxies are packed closely together, and their gravitational forces can lead to complex tidal interactions.

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SH2-91: A Supernova Remnant in Cygnus

SH2-91, located in the constellation Cygnus, is a fascinating supernova remnant lying about 6,000 light-years from Earth. This celestial object is the aftermath of a massive stellar explosion, where the outer layers of a dying star were ejected into space, creating a cloud of ionized gas and debris. The remnant is part of the Sharpless catalog of H II regions, though its nature as a supernova remnant distinguishes it from the more commonly known emission nebulae in this catalog.

SH2-91 is sometimes referred to as “The Other Veil in Cygnus”, because a much brighter and popular supernova remnant called the Veil Nebula also resides in Cygnus.

This particular image is a 5-panel mosaic and only captures a small portion of the entire faint structure. The supernova that created SH2-91 is thought to have occurred several thousand years ago, and the remnant’s structure is shaped by the shockwaves from the explosion. These shockwaves interact with surrounding gas and dust, creating a complex, expanding shell of material. SH2-91 is relatively faint and not immediately visible to the naked eye, but it can be detected in deeper observations, where it appears as a faint, diffuse glow.

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The Soap Bubble Nebula: A Planetary Nebula in Cygnus

Located about 4,700 light-years away in the constellation Cygnus, the Soap Bubble Nebula (not to be confused with NGC 7635 – The Bubble Nebula) is a fascinating and elusive structure within the larger star-forming region surrounding the Crescent Nebula. This faint and delicate nebula gets its name from its nearly spherical shape, resembling a cosmic soap bubble floating in space.

The Soap Bubble Nebula is the result of a stellar wind from a massive star, WR 136, which is also responsible for the Crescent Nebula nearby. This hot, young Wolf-Rayet star has been shedding its outer layers of gas and dust for millions of years, creating a bubble of ionized gas and dust that expands outward into space. The intense radiation from WR 136 lights up the surrounding gas, giving the nebula its faint, glowing edges.

What makes the Soap Bubble Nebula intriguing is its relatively small size and its dim, ghostly glow. Despite being a part of the more famous Crescent Nebula complex, the Soap Bubble remains a challenge to observe, requiring long exposures and advanced imaging techniques to capture its faint structure.

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Messier 81-82 (M81-M82): Bode’s Galaxy and the Cigar Galaxy Mosaic

Nestled within the constellation Ursa Major (the Great Bear) lies a notable pair of galaxies: M81 and M82.

Messier 81 (on the left), also known as M81 or NGC 3031, is a grand design spiral galaxy located about 11.8 million light-years away. It’s one of the brightest galaxies visible from Earth and is characterized by its well-defined spiral arms extending from a bright central nucleus.

Messier 82 (on the right), also known as M82 or NGC 3034, is a starburst galaxy situated about 12 million light-years away. Unlike M81, M82 exhibits a highly irregular and distorted shape due to intense gravitational interactions with its neighbor, M81. This interaction has triggered vigorous star formation, making M82 one of the brightest infrared sources in the sky.

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