NGC 2451 is a double cluster, consisting of the open clusters NGC 2451 A and NGC 2451 B, and they are located at around 600 and 1,200 light-years respectively. Naos, designated as Zeta Puppis, is the brightest star in the constellation of Puppis, and among the hottest, and most luminous stars visible to the naked eye, being the 72nd brightest star in the sky. Puppis stretches for around 673 square degrees. Zeta Puppis has been extensively studied because of its rareness and relative closeness to Earth, but its physical parameters and distance are still poorly known. The central star is possibly the hottest known white dwarf star, reaching temperatures of around 200,000 K, being 34.6 times hotter than our Sun, and 1,100 brighter. Image credit: Tahina Ramiaramanantsoa. It is located at around 1,600 light-years from us, and it has an apparent magnitude of 4.2. Zeta Puppis is a blue supergiant star of spectral class O5IAf, making it one of the hottest stars in the galaxy with a surface temperature of 42,400 K (in comparison, the Sun has a surface temperature of 5,780 K). Some of the notable deep-sky objects in Puppis are the Skull and Crossbones Nebula, NGC 2451, NGC 2477, Collinder 135, NGC 2438, NGC 2509, NGC 2439, NGC 2438, NGC 2440, NGC 2298, NGC 2546, or the Calabash Nebula, among others. It is particularly rich in open clusters, globular clusters, and nebulae since an important part of the Milky Way runs through this constellation. The constellation of Puppis is bordered by the constellations of Carina, Canis Major, Columba, Hydra, Monoceros, Pictor, Pyxis, and Vela. This open cluster is located at almost one degree away from Messier 46. It represents the stern of a ship, as it was once part of a larger constellation named the Argo Navis, which represented the mythical Argonauts. HD 60532 is a white F-type main-sequence star located at around 83.8 light-years away from us. It contains large amounts of sulfur, and the densest parts of the nebula are composed of a material ejected by the central star and accelerated in opposite directions. The constellation of Puppis is a southern constellation, that was once part of the great Argo Navis constellation, during Ptolemy’s era, as it was listed in the astronomer’s star catalog, named the Almagest, in the 2nd century. The Nine Planets has been online since 1994 and was one of the first multimedia websites that appeared on the World Wide Web. NGC 2298 is a globular cluster, and probably a former member of the Canis Major Dwarf galaxy. Zeta Puppis has been extensively studied because of its rareness and relative closeness to Earth, but its physical parameters and distance are still poorly known. The Zeta Puppids are a daylight meteor shower that takes place from May 20 to July 5, peaking on June 9 – 13. The Skull and Crossbones Nebula, designated as NGC 2467, is a star-forming region located at around 16,000 light-years away from us, in the constellation of Puppis. Currently, around 6 stars in the constellation of Puppis have been confirmed to host exoplanets. Zeta Puppis, also known as Naos, is a blue supergiant star, one of the most luminous stars in our Milky Way Galaxy. NGC 2477, also known as Caldwell 71, is an open cluster located at around 3,600 light-years away from us. The stars have apparent magnitudes of 5.52 (Zeta 1) and 5.22 (Zeta 2) and are visible to the naked eye from areas without light pollution. The star system is composed of two Sun-like stars, Zeta 1 and Zeta 2 Reticuli, located at a distance of about 39.3 light years from Earth. NGC 2439 is an open cluster that has an angular size of 10 arcminutes. Take an interactive tour of the solar system, or browse the site to find fascinating information, facts, and data about our planets, the solar system, and beyond. This planetary system is among the most similar to our own. This star is oblate since it has a rotational velocity of 238 km / 147.8 mi per second, leading to its equatorial radius to be 20% larger than its polar radius. L2 Puppis, also designated as HD 56096, is a giant star located at around 210 light-years away from us, between the bright star Canopus and Sirius. L2 Puppis is around 246 times bigger than our Sun, having only 60% of its mass, 12,300% of its radius while being around 2,000 times brighter than our Sun. Naos has an apparent magnitude of 2.25, and it is located at around 1080 light-years away from us. Asmidiske is cooler than our Sun, with temperatures reaching only 4,880 K. HD 70642 is a yellow dwarf star located at around 92 light-years away from us. Naos is more than 50 times bigger than our Sun, and it is 6.9 times hotter, with temperatures reaching 40,000 K. Naos is also a fast-spinning star, having a rotational velocity of 220 km / 136.7 mi per second. This cluster is 14 light-years wide, and it is around 1.2 billion years old. This cluster is 387.3 million years old, and it contains many bright, and variable stars. It has an apparent magnitude of 9.4. This globular cluster has an apparent magnitude of 9.3.

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