StarDate

A star system on the far side of the galaxy keeps blowing up. Since 1863, astronomers have recorded 12 outbursts from the system – the most recent just four years ago. The flare-ups are powered by a complicated interplay between a dead star and a companion that may be dying. U Scorpii probably is more than 60,000 light-years away, far on the other side of the heart of the Milky Way Galaxy. Most of the time, the system is quite faint. But during the outbursts, it can flare 10,000 times brighter in just a few hours. It starts to fade quickly, but it takes about two months to return to its “quiet” state. The system consists of two stars in a tight orbit. One of them is a white dwarf – the dead core of a Sun-like star. The other star is headed toward the same fate. It’s at the end of the prime phase of life, so it’s starting to puff up. The white dwarf “steals” some of the gas from its surface, forming a swirling disk. Some of the gas piles up on the white dwarf. Eventually, the gas gets so hot, it sets off a nuclear blast, making the system flare up. The outburst blows away all or part of the disk. Before long, though, the process starts all over again – leading to another explosion a few years later. U Scorpii is in Scorpius, which is low in the south-southeast at nightfall. The system is above the curving line of stars that outlines the scorpion’s body and tail. Script by Damond Benningfield

It’s hard to see a pattern in most of the constellations. Their stars are too faint or too spread out, or the pattern is just too obscure. Perhaps the most prominent exception is Scorpius. It takes little imagination to see the curving body of a scorpion in its stars. The scorpion skitters low across the south on summer nights. Its brightest star is Antares. The scorpion’s body and tail curl to the lower left. The head is to the upper right. It’s marked by a line of three stars. They’re about the same brightness, and they’re fairly evenly spaced. From top to bottom, the stars are Beta, Delta, and Pi Scorpii. Delta is a bit brighter than the others. All three stars are extraordinary. Each of them actually consists of more than one star. All of the member stars are quite young – no more than a few percent the age of the Sun. And most of them are big and heavy, with some of them fated to end their lives as supernovas – titanic explosions that will outshine billions of normal stars. Delta Scorpii consists of two stars. At least one of them will become a supernova. Pi Scorpii is a triple system. It also features at least one future supernova. Beta is the busiest of the systems – at least six stars, all orbiting each other in a complex gravitational ballet. Two of those stars are likely to become supernovas – briefly highlighting the head of the scorpion. Script by Damond Benningfield

Summer arrives here in the United States in the wee hours of tomorrow morning – the moment of the June solstice. At the solstice, the Sun stands farthest north for the entire year. For people at about 23-and-a-half degrees north latitude, our star will pass directly overhead at local noon. That line of latitude is known as the Tropic of Cancer. It was named a couple of thousand years ago. At the time, the Sun appeared against the constellation Cancer at the solstice. Today, though, the Sun’s almost directly astride the border between Taurus and Gemini. It’s on the Taurus side at the exact moment of the solstice, but it slides into Gemini a few hours later. The change in address is the result of a slow “wobble” in Earth’s axis. As it wobbles, the Sun shifts position against the background of stars. It takes our planet about 26,000 years to complete a single wobble, so that’s how long it takes the Sun to move all the way across the zodiac. So the Sun will return to Cancer in about 24,000 years. Earth’s axis also nods up and down a little over an even longer period – about 41 thousand years. That causes a shift in the latitude of the Tropic of Cancer. Right now, it’s moving southward at about 50 feet per year – changing the circle where the Sun stands overhead on the summer solstice. We’ll have more about the summer solstice tomorrow. Script by Damond Benningfield

Like a cosmic butterfly, a cluster of young stars is just emerging from its cocoon – a cloud of gas and dust. The cocoon `spans about 45 light-years. But some of the beautiful butterfly is already in view. Parts of the gas cloud are lit up by the brightest of the infant stars taking shape there. That creates a glowing patch of red and blue. The whole complex is known as the Cocoon Nebula. It’s about 4,000 light-years away, in Cygnus. Hundreds of stars are being born inside it. The most impressive of those stars is about 14 times as massive as the Sun, and tens of thousands of times brighter. It’s especially bright in the ultraviolet – wavelengths that are invisible to the human eye. The U-V zaps atoms of hydrogen in the nebula, splitting them apart. When the atoms re-combine, they emit red light – the main color of the nebula. The hot star also illuminates dust grains in the nebula. It doesn’t set them aglow; instead, the light simply reflects off the grains. That colors the blue parts of the nebula. Less-massive stars – stars like the Sun or even smaller – are still coming together. They won’t shine as fully formed stars for millions of years. The Cocoon Nebula is low in the northeast at nightfall. It’s to the lower left of the bright star Deneb, which marks the tail of the swan. The nebula is too faint to see with the eye alone. Script by Damond Benningfield