A Flare for Barnard's Star

By Ken Croswell

Published on Astronomy.com (November 11, 2005).

Barnard's Star, the second nearest star system to the Sun, spewed a large flare that increased its brightness, say astronomers in the United States. The discovery is a surprise: the star should be sedate, because it's an old red dwarf.

Red dwarfs are smaller, cooler, and fainter than the Sun. When young and middle-aged, they often spin fast enough to generate strong magnetic fields. These cause flares that can double the star's brightness in just a few seconds.

As red dwarfs age, they spin more slowly. Barnard's Star is old, a likely member of the Milky Way's thick-disk population. Its age is probably 11 or 12 billion years, which is more than twice the Sun's age. And small periodic variations in the star’s light suggest it rotates slowly, only once every 130 days. Thus, the star should not emit flares.

However, Diane Paulson of NASA's Goddard Space Flight Center in Greenbelt, Maryland, and her colleagues report Barnard's Star unleashed a flare July 17, 1998. At the time, William Cochran of the University of Texas at Austin was using McDonald Observatory's 2.7-meter telescope to obtain the star's spectrum. He hoped to detect changes that signified orbiting planets. Instead, he noticed emission lines in the spectrum that indicated the star might be flaring, and he obtained two additional spectra that night. But because he was interested in planets rather than flares, he did not pursue the matter further.

Four years later, Cochran showed the spectra to Paulson, then a graduate student in Austin. Her team's recent analysis indicates that despite the star's old age, its hot blue flare resembled those from younger red dwarfs. The flare's temperature was at least 8,000 Kelvin, more than double the star's temperature of 3,100 Kelvin.

Unfortunately, spectra can't determine just how much Barnard's Star brightened that night. Paulson estimates the rise at visual wavelengths was half a magnitude or more. The flare lasted at least an hour.

"The star would be fantastic for amateurs to observe," says Paulson. Located in northern Ophiuchus, Barnard's Star is magnitude 9.55. Amateur observers can easily monitor its brightness and search for future flares. As the astronomers write, however, "Because Barnard's star is considered to be one of our oldest neighbors, a flare of this magnitude is probably quite rare."

American astronomer Edward Emerson Barnard discovered Barnard's Star in 1916. It has a large proper motion--the greatest of any star--which results both from the star's high speed through space and from its proximity to Earth. Precise parallax data from the Hubble Space Telescope indicate it is 5.98 light-years away, making it the second closest star system to the Sun. Only the triple star Alpha Centauri is nearer.

The new discovery means all three of the three nearest red dwarfs are flare stars: Proxima Centauri, the faintest member of the Alpha Centauri system; Barnard's Star; and Wolf 359 in Leo, which is 7.8 light-years from Earth. However, Proxima Centauri and Wolf 359 are sufficiently active that their flares were found more than half a century ago.

Paulson and her colleagues will publish their work in a future issue of Publications of the Astronomical Society of the Pacific.

Ken Croswell is an astronomer and the author of Magnificent Universe and See the Stars: Your First Guide to the Night Sky.

"Elegant and eloquent"--Washington Post. See all reviews of Magnificent Universe here.

"Finally! An astronomy guide that the reader can actually follow without being a rocket scientist!" See all reviews of See the Stars here.

BARNARD'S STAR AND THE SUN

	Barnard's Star	The Sun
Constellation	Ophiuchus	---
Distance (light-years)	5.98	---
Apparent Magnitude	9.55	-26.74
Absolute Magnitude	13.23	+4.83
Relative Brightness	0.00044	1.00
Spectral Type	M4	G2
Color	Red	Yellow
Temperature	3100 K	5770 K
Relative Mass	0.16	1.00
Relative Radius	0.20	1.00
Proper Motion (arcseconds/year)	10.51	---
Radial Velocity (kilometers/second)	-111	---

THE THREE LARGEST-PROPER-MOTION STARS

Star	Constellation	Distance	Spectral	App. Mag.	Abs. Mag.	Discoverers	Year	Proper Motion
		(light-years)	Type					(arcsec/year)
Barnard's Star	Ophiuchus	5.98	M4	9.55	13.23	Edward Emerson Barnard	1916	10.51
Kapteyn's Star	Pictor	12.8	M1	8.84	10.87	Jacobus Kapteyn/Robert Innes	1897	8.66
Groombridge 1830	Ursa Major	30	G8	6.45	6.64	Friedrich Argelander	1841	7.06

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