Gliese 250 is another binary star in Monoceros. It is approximately 489 light years distant from the Sun. It is the brightest visible star in Monoceros. The star is twice as luminous as the Sun and has 18 percent more mass. You can decline to give a name which if that is the case, the comment will be attributed to a random star. The brightest star has around 2,910% of our Sun’s mass, 990% of its radius, and it is a whopping 214,000 times brighter. Cookies / About Us / Contact Us / Twitter / Facebook, Bet Mon, HD 45725, HIP 30867, HR 2356, TYC 4797-1882-1, 11 Monocerotis, 11 Mon, 06 1574, NSV 02977, Variable Magnitude Range (Brighter - Dimmer), Beta Monocerotis is a main star in the constellation.

Information regarding Metallicity and/or Mass is from the E.U. At low power, it appears to be a double star, but bumping up the magnification shows the eastern component to be a close double itself. Monoceros is the 35th constellation in size, occupying an area of 482 square degrees. NGC 2232 has an apparent magnitude of 3.9, and it is among the nearest open clusters to the Solar System, having around 100 solar masses, and a radius of about 15 light-years. Apparent Magnitude is also known as Visual Magnitude. Monoceros contains two formally named stars. This along with Camelopardalis was created by Jakob Bartsch and there is no Greek mythology behind it. If the R.A. is positive then its eastwards. to have found Monoceros on an ancient Persian sphere.

They have luminosities 20 and 2.5 times that of the Sun, radii 2.2 and 1.2 times solar, and masses 1.9 and 1.25 times that of the Sun. Image: NASA and the Hubble Heritage Team. It belongs to the stellar class G9V. The constellation represents the mythical single-horned, horse-like creature.

The visual magnitudes of the stars are 4.7, 5.2, and 6.1. It acquired its moniker because of its shape and its apparent colour when seen in early images from Earth. Monoceros belongs to the Orion family of constellations, along with Canis Major, Canis Minor, Lepus and Orion. It has a total mass about 100 times that of the Sun. It consists of two stars that cannot be resolved, that orbit each other with a period of 25 years.

The figure is derived at by using the formula from SDSS rather than peer reviewed papers.
Its surface temperatures have been estimated at around 44,000 K, more than 7 times as hot as our Sun. The B component is also a very fast-spinning star, having a rotational velocity of around 300 km / 186.4 mi per second. NGC 2264 is a New General Catalogue designation for two deep sky objects – the Christmas Tree Cluster and the Cone Nebula – and there are two other objects that fall within this designation, but are not officially included: the Snowflake Cluster and the Fox Fur Nebula. Ross 614 a red dwarf star classified as a UV Ceti type variable, which means that it is a type of flare star. They all belong to the spectral class B3 and have temperatures around 18,500 K. They are all hydrogen-fusing dwarfs. Scholtz is named after the scientist who studied or led the study into it, Ralf-Dieter Scholz in 2013. You also have the option to opt-out of these cookies. The brightest star in the constellation is Beta Monocerotis, with an apparent magnitude of 3.76. The best time to observe stars and deep-sky objects in the constellation of Monoceros is during the month of February. It is approximately 2,000 light years distant. It is an H II region positioned near a large molecular cloud. The constellation of Monoceros hosts numerous interesting deep-sky objects, such as the Rosette Nebula, the Christmas Tree Cluster, the Cone Nebula, Hubble’s Variable Nebula, and the reflection nebula IC 447 among others.

[9], German astronomers Heinrich Wilhelm Olbers and Ludwig Ideler[10] Monoceros is quite faint since it doesn’t have any stars brighter than magnitude 3.0. The second biggest star in this system has 2,130% of our Sun’s mass.
Granted, V616 Monoceros is not a star but it is dead remnants of a giant star. Zeta Monocerotis is a massive, luminous, yellow supergiant star in Monoceros.

U.G.


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