The Vega system may be somewhat like a scaled-up version of our own solar system, as shown in this diagram. Astronomers have discovered a band of warm dust close to the star, and a band of colder material farther out. Planets may inhabit the space between them. The solar system is shown both to scale (bottom) and enlarged to the same size as the Vega system. [NASA/JPL/Caltech]
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The second-brightest star in the northern half of the sky is in great view as we head toward summer. Vega is well up in the east-northeast as darkness falls, and climbs high overhead later on.
Vega is a bit like a scaled-up version of the Sun — it’s more than twice the Sun’s diameter and mass. And it’s encircled by scaled-up versions of the belts of comets and asteroids that surround the Sun. That suggests it could have a scaled-up planetary system as well.
Space telescopes have mapped the debris around Vega in detail — bits of dust, rock, and ice that glow at infrared wavelengths.
By studying the observations, astronomers determined that Vega has a ring of dust and rock that resembles the asteroid belt in our own solar system. They also found that there’s a larger ring of cold material much farther from Vega. That ring resembles the Kuiper Belt — a broad band of icy bodies beyond the orbit of Neptune, the Sun’s most distant major planet.
The Vega system is about four times wider than the solar system. But if you scaled up the solar system, those belts of debris would look almost identical.
In the solar system, there are four planets between the Sun and the asteroid belt, and four more between the asteroid belt and the Kuiper Belt. No one has yet found any planets orbiting Vega. But the presence of the debris suggests that planets could be orbiting the star — clearing out wide zones between Vega’s “dusty” belts.
Script by Damond Benningfield