Barnard’s Star is a red dwarf about six light-years away from Earth in the constellation of Ophiuchus. It is the fourth-nearest-known individual star to the Sun after the three components of the Alpha Centauri system, and the closest star in the northern celestial hemisphere. Despite its proximity, the star has a dim apparent magnitude of +9. 5 and is invisible to the unaided eye; it is much brighter in the infrared than in visible light.
About Barnard’s Star in brief

At 7–12 billion years of age, Barnard’s Star is considerably older than the Sun, which is 4. 5 billion years old. It might be among the oldest stars in the Milky Way galaxy. It was long assumed to be quiescent in terms of stellar activity, but in 1998, astronomers observed an intense stellar flare, showing it is a flare star. The proper motion of Barnards Star corresponds to a relative lateral speed of 90 kms. The 10.3 seconds of arc it travels annually amount to a quarter of a degree in a human lifetime, roughly half the angular diameter of the full Moon. The effective temperature is 3,100 kelvin and it has a visual luminosity of 0. 0004 solar luminosities. Its mass is about 150 times the mass of Jupiter, although its radius is only about 1 5 to 2 times larger, due to its much higher density. The Sun will still be seen with the naked eye yet, since its apparent magnitude will only have increased by one magnitude to about 8. 5 by then, still being short by 2 magnitudes of visibility by then by then. The Star has a mass of 14 solar masses and a radius of 15% to 20% of that of the Sun. It rotates once in 130 days, and its rotational energy is about 1.5 times the radius of Jupiter, although its mass is only 1.2 times that of Jupiter.
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This page is based on the article Barnard’s Star published in Wikipedia (as of Nov. 22, 2020) and was automatically summarized using artificial intelligence.






