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Summer Triangle Corner: Vega<\/h1>\n<\/div>\n<\/div>\n<\/div>\n
If you live in the Northern Hemisphere and look up during July evenings, you\u2019ll see the brilliant star\u00a0Vega<\/strong>\u00a0shining overhead. Did you know that Vega is one of the most studied stars in our skies? As one of the brightest summer stars, Vega has fascinated astronomers for thousands of years.<\/p>\n Vega is the brightest star in the small Greek constellation of Lyra, the harp. It\u2019s also one of the three points of the large \u201cSummer Triangle\u201d asterism, making Vega one of the easiest stars to find for novice stargazers. Ancient humans from 14,000 years ago likely knew Vega for another reason: it was the Earth\u2019s northern pole star! Compare Vega\u2019s current position with that of the current north star<\/a>, Polaris, and you can see how much the direction of Earth\u2019s axis changes over thousands of years. This slow movement of axial rotation is called\u00a0precession<\/a><\/strong>, and in 12,000 years, Vega will return to the northern pole star position.<\/p>\n Bright Vega has been observed closely since the beginning of modern astronomy and even helped to set the standard for the current magnitude scale used to categorize the brightness of stars. Polaris and Vega have something else in common, besides being once and future pole stars: their brightness varies over time, making them\u00a0variable stars<\/strong>. Variable stars\u2019 light can change for many different reasons. Dust, smaller stars, or even planets may block the light we see from the star. Or the star itself might be unstable with active sunspots, expansions, or eruptions changing its brightness. Most stars are so far away that we only record the change in light, and can\u2019t see their surface.<\/p>\n NASA\u2019s TESS satellite has ultra-sensitive light sensors primed to look for the tiny dimming of starlight caused by transits of extrasolar planets. Their sensitivity also allowed TESS to observe much smaller pulsations in a certain type of variable star\u2019s light than previously observed. These observations\u00a0of Delta Scuti\u00a0<\/strong>variable stars will help astronomers model their complex interiors and make sense of their distinct, seemingly chaotic pulsations. This is a major contribution towards the field of astroseismology<\/strong>: the study of stellar interiors via observations of how sound waves \u201csing\u201d as they travel through stars. The findings may help settle the debate over what kind of variable star Vega is. Find more details on this research, including a sonification demo that lets you \u201chear\u201d the heartbeat of one of these stars, at:\u00a0bit.ly\/DeltaScutiTESS<\/a> Originally posted by Dave Prosper: June 2020 Powered by WPeMatico<\/a><\/small><\/p>\n Get The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" If you live in the Northern Hemisphere and look up during July evenings, you\u2019ll see the brilliant star\u00a0Vega\u00a0shining overhead. Did you know that Vega is one of the most studied stars in our skies? As one of the brightest summer stars, Vega has fascinated astronomers for thousands of years.Vega is the brightest star in the [\u2026] Continue reading ![\"The](\"https:\/\/assets.science.nasa.gov\/dynamicimage\/assets\/science\/cds\/nightsky\/articles\/Summer%20Triangle%20005.jpeg?w=1259&h=945&fit=clip&crop=faces%2Cfocalpoint\")
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In 2024, the James Webb Space Telescope revisited the Vega system to reveal a 100-billion-mile-wide disk of dust<\/a> around this star. While the debris disk is confirmed, there is no evidence of planets as of today.<\/p>\n
Last Updated by Kat Troche: July 2025<\/em><\/p>\n