StarDate

Billy Henry

StarDate, the longest-running national radio science feature in the U.S., tells listeners what to look for in the night sky.

Episodios

  1. HACE 2 D

    Moon and Antares

    A future super-giant “onion” perches close to the Moon at dawn tomorrow. It’s the star Antares, the bright heart of the scorpion – one of the most impressive stars in the galaxy. Antares is a supergiant. It’s roughly a dozen times as massive as the Sun, and hundreds of times wider. Because it’s so heavy, gravity squeezes its core tightly. That revs up the nuclear fusion in the core. Like all stars, those reactions initially fused hydrogen to make helium. In the Sun, hydrogen fusion will last about 10 billion years. In Antares, though, it lasted a little more than 10 million years. When the hydrogen in the core was gone, the core shrank, making it hotter – hot enough for the helium to fuse to make carbon and oxygen. That process will last about one million years. Then the carbon will fuse to make heavier elements, and so on. Each step takes less time than the one before. In the final step, silicon will fuse to make iron – a step that takes just a few days. The lighter elements won’t all go away, though. Instead, the “ash” from each step will form layers around the core – like an onion. But that structure won’t last. The core can’t get hot enough to fuse the iron. Gravity will win out, and the core will collapse – forming an ultra-dense neutron star. Everything outside the core will blast outward at a few percent of the speed of light. Supergiant Antares will explode as a supernova – an impressive end for an impressive star. Script by Damond Benningfield

    2 min
  2. HACE 3 D

    Bad Neighbor

    Canopus would be a terrible neighbor. The star is big, bright, and hot, so it might blow away any planet-making materials around nearby stars. Even worse, it may be destined to explode. That would zap any existing planets with radiation – perhaps endangering any life in nearby star systems. Canopus is the second-brightest star in the night sky. At this time of year, it’s visible from the southern third of the United States in early evening. It’s low in the south, well below Sirius, the brightest star. Canopus is at least eight times the mass of the Sun. So even though it’s billions of years younger than the Sun, it’s already completed the main phase of life. Within a few million years, its core will collapse, perhaps forming an ultra-dense neutron star. If so, then its outer layers will blast into space as a supernova. Such an outburst would produce enormous amounts of X-rays and gamma rays – the most powerful forms of energy. That could strip away the ozone layer of any planet within a few dozen light-years, subjecting the surface to high levels of radiation. So far, we know of only one planet within that range where conditions are most suitable for life. The planet itself isn’t likely to host life. But any big moons might be more comfortable homes – at least until the demise of Canopus. Luckily for us, Canopus is 300 light-years away. So Earth is well outside the “danger zone” of this not-so-neighborly neighbor. Script by Damond Benningfield

    2 min
  3. 4 MAR

    Long Death Cry

    Last July, a space telescope heard the death cry of a star billions of light-years away. It was the longest outcry of its type ever detected – an astonishing seven hours. Yet its details are still fuzzy. All we know for sure is that it was a violent ending for a star. The outcry was a gamma-ray burst. Astronomers have discovered thousands of them. They’re usually produced by a supernova – the titanic explosion of a massive star. Energy from the nuclear inferno deep inside the star blasts outward through its poles. That forms narrow jets of gamma rays – the most powerful form of energy. The gamma rays usually last a few seconds or minutes. In that time, though, the burst can emit more energy than the Sun will produce over billions of years. Follow-up observations showed that the July outburst took place in a galaxy that’s giving birth to many stars – perhaps as the result of a merger with another galaxy. Many of the new stars are hot and massive, so they explode quickly. That makes the galaxy a good breeding ground for gamma-ray bursts. But the origin of this event isn’t clear. It could have been the result of a supernova. Other possible scenarios include the merger of a black hole with the dead or stripped core of a Sun-like star, or a close encounter between a star and a mid-sized black hole. Such an encounter would have ripped the star apart, forming a trail of incandescent gas – triggering a long outcry from a dying star. Script by Damond Benningfield

    2 min
  4. 3 MAR

    Venus and Saturn

    Two of the planets of the solar system are crossing paths in the early evening. But they’re quite low in the sky, so they can be a bit tough to spot. The brighter of the two is Venus, which is beginning its reign as the “evening star.” It’ll climb higher into the sky over the coming weeks and months, making it much easier to spot. Right now, though, it sets by the time the color of twilight drains away, so there’s not much time to enjoy it. Venus’s companion is Saturn. It’s close to the upper left of Venus. It’s only about one percent as bright, so it’s tougher to pluck from the twilight. You might miss it entirely if not for the presence of its brighter sibling. And the two planets really are siblings. They were born from the same cloud of gas and dust that surrounded the newborn Sun. Venus was born close to the Sun. Conditions in that region were so hot that only heavier materials were available to build planets. So, like Earth, Venus is made mostly of rock and metal. Saturn took shape in the deep-freeze of the outer solar system. The planet built a big core of heavy materials. The core then pulled in huge amounts of gas. That made Saturn the second-largest planet – a cold, gassy world far from the Sun. Watch Venus and Saturn as they cross paths the next few nights. They’ll stand side by side on Saturday, just a whisker apart. Venus will pull away after that, with Saturn vanishing in the sunlight. Script by Damond Benningfield

    2 min
  5. 1 MAR

    Moon and Regulus

    The Moon stalks the heart of the lion tonight. And seen from Hawaii, it’ll catch it. The Moon will “occult” the heart, blocking it from view. The lion’s heart is Regulus, the brightest star of Leo. The name Regulus means “the little king.” It was introduced 500 years ago. But the star’s association with royalty goes back much farther. In ancient Persia, Regulus was one of the four “royal” stars – four especially bright stars near the ecliptic – the Sun’s path across the sky. The stars are roughly evenly spaced around the ecliptic. That means each star is at its best during a different season. So each star was considered the “guardian” of its season. Regulus is closer to the ecliptic than the other three guardians, so it was the most important of them all – a king among kings. The Moon stays close to the ecliptic as well, straying only a few degrees to either side. So it circles past the same stars every month – including Regulus. Right now, the Moon’s path carries it especially close. And that’s easy to see tonight. Regulus is below the Moon as night falls. But as the hours roll by, the Moon will creep closer and closer to the bright star. As seen from the continental United States, they’ll be separated by no more than about one degree as they set, before dawn – the width of a pencil held at arm’s length. And from Hawaii, the Moon will catch the star – “eclipsing” the little king. Script by Damond Benningfield

    2 min

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StarDate, the longest-running national radio science feature in the U.S., tells listeners what to look for in the night sky.

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