No. R136a1 is in the Tarantula Nebula, in the Large Magellanic Cloud, in the constellation Dorado
T Tauri is a variable star in the constellation Taurus that is a young, pre-main-sequence star. An example of a T Tauri star is T Tauri itself, which is located in the Taurus-Auriga star-forming region and is surrounded by a protoplanetary disk. These stars are characterized by strong magnetic fields, irregular variability, and intense stellar winds.
R136a1 is a blue hypergiant star located in the Large Magellanic Cloud. It is estimated to be approximately 265 times the mass of our Sun, making it one of the most massive stars known in the universe.
R136a1 is one of the hottest known stars, with surface temperature around 50,000 degrees Celsius (90,000 degrees Fahrenheit). Its extreme heat causes it to emit intense ultraviolet radiation and it is a supergiant star, approximately 250 times more massive than the sun.
T Tauri is a variable star in the constellation Taurus.Unfortunately, there is no data at the moment as to it's size, probably because of the amount of stellar material still orbiting it.
The dividing line is usually considered to be when the accretion process stops and the T tauri wind begins. This is probably approximately coincident with the beginning of lithium fusion (a T tauri star is not yet hot and dense enough for hydrogen fusion to start).
Yes. Zeta Tauri, Kappa Tauri, and Lambda Tauri are eclipsing binary stars.
Tauri Tiido goes by Tiido.
Epsilon Tauri b was created in 2007.
Tauri Tiido was born on December 19, 1992, in Tartu, Estonia.
R136a1's heat would probably vaporize all of the planets.
r136a1
T Tauri is a variable star in the constellation Taurus that is a young, pre-main-sequence star. An example of a T Tauri star is T Tauri itself, which is located in the Taurus-Auriga star-forming region and is surrounded by a protoplanetary disk. These stars are characterized by strong magnetic fields, irregular variability, and intense stellar winds.
As far as mass goes, R136a1 beats out VY Canis Majoris by 253 solar masses (265 solar masses for R136a1 vs Canis Majoris' 30). However, VY Canis Majoris beats out R136a1 in radius by about 1,385 solar radii (Canis Majoris is 1,420 solar radii vs R136a1's ~35).
Zeta Leonis Epsilon Canis Majoris Epsilon Tauri Eta Lyrae Gamma Andromedae Mu Lyrae Beta Virginis Pi Sagittarii Epsilon Aquarii Beta Cygni Alpha Corvi 80 Ursae Majoris
The T Tauri wind is a stream of charged particles emitted by a young, newly formed T Tauri star. These winds are powerful and can impact the surrounding environment, influencing the dynamics of the protoplanetary disk and potentially affecting the formation of planets in the system.
R136a1 is a blue hypergiant star located in the Large Magellanic Cloud. It is estimated to be approximately 265 times the mass of our Sun, making it one of the most massive stars known in the universe.
T-Tauri phasee