$0.00
Emission nebula NGC 249
Prints
Discovered in 1826 by the illustrious astronomer James Dunlop. NGC 249 is a captivating emission nebula (a cloud of high temperature gas) situated in the Tucana constellation. This astronomical marvel was first observed on September 5, 1826, by the renowned astronomer James Dunlop. NGC 249 is situated south of the celestial equator, and, as such, it is more easily visible from the southern hemisphere.
As an emission nebula, NGC 249 is a region of ionized gas emitting light of various wavelengths, offering a spectacular view in the realm of deep space. Its discovery by Dunlop marks a significant moment in the study of celestial bodies, contributing to our understanding of the complex and beautiful phenomena in our universe.
Also in Prints
M45 Pleaides Star Cluster
$0.00Pleiades and Orion are both constellations in the Bible, not people. They are referenced to provide a scope to the power and ability of God as a creator who made everything, even the stars in the sky above. Pleiades is a cluster of stars, part of the constellation Taurus. It is also known as the Seven Sisters.
IC 1396 Elephants Trunk Nebula
$0.00The Elephant's Trunk Nebula, designated as IC 1396A, is a concentration of interstellar gas and dust within the larger emission nebula IC 1396. Located in the constellation Cepheus, this nebula is approximately 2,400 light-years away from Earth. The Elephant's Trunk Nebula gets its name due to its elongated shape, resembling the trunk of an elephant.
M27 Dumbbell Nebula
$0.00The M27 Dumbbell Nebula, also known as Messier 27 or NGC 6853, is one of the most famous and frequently observed planetary nebulae in the night sky. Located approximately 1,360 light-years away in the constellation Vulpecula, it was the first planetary nebula ever discovered, identified by Charles Messier in 1764.
The Dumbbell Nebula gets its name from its distinctive shape, which resembles a dumbbell or an hourglass when viewed through a telescope. This shape is created by the expanding shell of ionized gas ejected from a dying star at the nebula's center. As the star expels its outer layers, it forms a glowing cloud of gas that is illuminated by the remaining hot core of the star, now a white dwarf.
With its intricate structure and vivid colors, the Dumbbell Nebula is a popular target for amateur astronomers and astrophotographers. The nebula's appearance can vary depending on the wavelength of light in which it is observed, often displaying hues of red and green due to the ionized hydrogen and oxygen gases. Observing the Dumbbell Nebula offers a glimpse into the final stages of a star's life cycle and the ongoing processes of stellar evolution.
NGC 6888 Crescent Nebula
$0.00The Crescent Nebula, also known as NGC 6888, is an emission nebula formed by the powerful stellar winds from its central star, WR 136. This Wolf-Rayet star is nearing the end of its life, shedding its outer layers and creating the beautifully complex and bright structure we see today. The interplay of glowing gases and dust creates a vivid tapestry of reds and blues, making it a favorite target for astrophotographers.
Rosette Nebula
$0.00The Rosette Nebula, a vast region of ionized hydrogen gas located in the Monoceros constellation, is an emission nebula distinguished by its rose-like appearance. This celestial structure is approximately 5,000 light-years from Earth and spans about 130 light-years in diameter. At the heart of the Rosette Nebula lies the open star cluster NGC 2244, whose young, hot stars emit intense ultraviolet light, ionizing the surrounding gas and causing the nebula to glow. The nebula's intricate shapes and patterns are sculpted by the stellar winds and radiation from these stars, making it a fascinating subject for astrophotography.