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Stars in JADES-GS-z14-0: 2024 z= 13.27 13.6 Gly (light travel distance) 34 Gly (proper distance) [5] List of the most distant astronomical objects: Most distant star gravitationally bound to Milky Way galaxy ULAS J0015+01: 2014 900,000 light-years Located in the Milky Way's extreme outer halo, far beyond the galactic disc. [6] Oldest star
List of the largest known stars in the Milky Way Star name Solar radius (R ☉) Method [a] Notes Orbit of Saturn: 2,047 – 2,049.9 [10] [b] Reported for reference: Theoretical limit of star size (Milky Way) ≳1,700 [11] L/T eff: Estimated by measuring the fraction of red supergiants at higher luminosities in a large sample of supernova ...
Sh2-310 is also host to the stars Tau Canis Majoris [35] which is the brightest member of NGC 2362, [36] UW Canis Majoris and HD 58011 [35] which along with VY Canis Majoris [37] are thought to be probable sources of ionization of gases in Sh2-310. [35] Sh2-310 itself is located on the outer edge of the Orion Arm of the Milky Way. [32]
The disk of stars in the Milky Way does not have a sharp edge beyond which there are no stars. Rather, the concentration of stars decreases with distance from the center of the Milky Way. Beyond a radius of roughly 40,000 light years (13 kpc) from the center, the number of stars per cubic parsec drops much faster with radius. [120]
The mass is equally uncertain, thought to have been up to 200 times the Sun when initially formed but now considerably less due to extreme mass loss although likely still over 100 times the Sun. [10] Modelling the star itself to match its spectrum gives a mass of 27.5 M ☉, [7] while matching its current properties to an evolutionary model ...
The Gaia Sausage or Gaia Enceladus is the remains of a dwarf galaxy (the Sausage Galaxy, or Gaia-Enceladus-Sausage, or Gaia-Sausage-Enceladus) that merged with the Milky Way about 8–11 billion years ago. At least eight globular clusters were added to the Milky Way along with 50 billion solar masses of stars, gas and dark matter. [1]
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. [7] At a distance of around 50 kiloparsecs (163,000 light-years), [2] [8] [9] [10] the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (c. 16 kiloparsecs (52,000 light-years) away) and the possible dwarf irregular galaxy called the Canis Major Overdensity.
A high-velocity star travelling the Milky Way at 456 km/s. [113] Gliese 1002: 95,310 Has two confirmed exoplanets [114] LHS 1070 A 97,400 [81] LHS 3154: 97,400 Has one confirmed exoplanet [115] Wolf 424 B 97,400 [116] Wolf 359: 100,180.8: Fifth-nearest star system to the Solar System. Has one unconfirmed exoplanet [105] NN Serpentis red dwarf ...
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