Best Puppis
Naos, formally designated Zeta Puppis, is a blue O-type supergiant star located in the constellation Puppis. It is one of the hottest, most luminous, and most massive stars visible to the naked eye, possessing a surface temperature of approximately 42,000 Kelvin. The star is situated roughly 1,000 l...
The Calabash Nebula, formally designated OH 231.8+4.2, is a protoplanetary nebula located in the constellation Puppis at a distance of roughly 4,200 light-years from Earth. It is also referred to as the Rotten Egg Nebula due to the unusually high concentration of sulfur compounds detected in its che...
The Rotten Egg Nebula, formally designated OH 231.8+4.2, is a bipolar nebula within the Puppis constellation. It’s notable for its high sulfur content and the powerful jets of gas emanating from QX Puppis, a young proto-planetary object at its center. Astronomers study this nebula to understand proc...
NGC 2440 is a planetary nebula located within the constellation Puppis. It’s recognized for its intricate, multi-lobed structure formed by the outflow of gas from a dying star. At its center lies a white dwarf emitting intense heat, reaching temperatures approaching 200,000 Kelvin. Astronomers and r...
NGC 2467 is a vibrant emission nebula located within the Puppis constellation. It represents a complex star-forming region characterized by a dense cluster of young, hot stars. These massive stars intensely illuminate surrounding gas and dust, creating the nebula’s distinctive glow. Astronomers and...
The Calabash Nebula, formally designated OH 231.8+4.2, is a bipolar protoplanetary nebula within the Puppis constellation. It’s notable for its distinctive shape and intense outflows of sulfur-rich gas, remnants from a dying star's outer layers. Astronomers study this object to understand the proces...
CG 4, nicknamed God's Hand, is a cometary globule in the constellation Puppis, notable for its faint, finger-like extensions of interstellar dust.
The Skull and Crossbones Nebula, designated as NGC 2467, is a star-forming region located in the southern constellation of Puppis. It is characterized by its distinct visual appearance, which loosely resembles a human skull and crossbones when viewed through long-exposure astrophotography. The nebul...
Puppis A is a supernova remnant located in the northern part of the constellation Puppis, approximately 7,000 light-years from Earth. The explosion that created the nebula is estimated to have occurred roughly 3,700 years ago, and the expanding cloud of gas continues to glow in X-ray and radio wavel...
NGC 2467, commonly known as the Skull and Crossbones Nebula, is an H II region and active star-forming area in the constellation Puppis. First recorded by William Herschel in 1784, this emission nebula contains young, hot stars that illuminate the surrounding gas clouds. The nebula's distinctive app...
Tureis, formally designated Rho Puppis, is a pulsating variable star located in the southern constellation of Puppis. It is categorized as a Delta Scuti variable, meaning its brightness fluctuates slightly over a period of a few hours due to radial pulsations. The star is an F-type bright giant situ...
NGC 2467 is an active star-forming region located in the southern constellation of Puppis. The nebula consists of bright emission clouds interspersed with dark dust lanes, creating an appearance that has led to its unofficial nickname, the Skull and Crossbones. It serves as a rich area for astronomi...
Sh2-311 is a large emission nebula and H II region in the constellation Puppis, also identified with NGC 2467. Its glowing gas is ionized by young, hot stars, and the surrounding complex contains active star formation, dark dust structures, and the young stellar groups Haffner 18 and Haffner 19. Inf...
NGC 2438 is a planetary nebula in the constellation Puppis that appears within the boundaries of the open cluster Messier 46 when viewed from Earth. Measurements of its motion and distance indicate that the nebula is not physically associated with the cluster, making the pairing a line-of-sight coin...
A bipolar protoplanetary nebula in Puppis named for its unusually high sulfur compound content, with opposing gas jets expanding at over 400 km/s into the surrounding interstellar medium.
A supernova remnant in Puppis roughly 7,000 light-years away, estimated to have exploded about 3,700 years ago and one of the brightest sources of X-ray and radio emission in the sky.
