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.

单集

  1. 1天前

    Event Horizon

    For a trip that’s out of this universe, just cross the event horizon of a black hole. Nothing that passes through an event horizon can ever come back out, so we don’t really know what goes on inside a black hole. But we can be pretty sure that it’s like nothing else in the universe. A black hole’s mass is concentrated in a single point, called a singularity. Its gravity is infinitely strong. But as the distance from the singularity increases, its grip weakens. Eventually, it reaches a point where the escape velocity equals the speed of light – the event horizon. Since nothing can travel faster than light, anything that falls through the horizon is trapped. It may be doomed to merge with the singularity. So the event horizon acts like the “surface” of a black hole. But it’s not solid – there’s nothing to ram into. Instead, it’s more of a boundary between the black hole and anything outside it. The distance between the singularity and the event horizon marks the size of the black hole. And as more stuff falls in, the black hole gets bigger. A black hole that’s 10 times the mass of the Sun spans about 35 miles. The supermassive black hole at the heart of the Milky Way spans 13 million miles. And the heaviest black holes yet seen are more than 40 times the size of the orbit of Neptune, the Sun’s outermost major planet – a wide entrance to an out-of-this-universe experience. More about black holes tomorrow. Script by Damond Benningfield

    2 分钟
  2. 3天前

    Moon and Antares

    Antares has played a big role in the skylore of many cultures. And it’s not hard to understand why. It’s quite bright, it has a fiery orange color, and it’s near the ecliptic – the Sun’s path across the sky. The Moon and planets are close to the ecliptic as well, so they periodically swing past Antares. In fact, the Moon snuggles quite close to it late tonight. In western skylore, Antares represented the heart of Scorpius, the scorpion. After Orion the hunter bragged that he could kill any beastie on Earth, the angry gods sent the scorpion to sting him to death. They then put Orion and the scorpion on opposite sides of the heavens, so one rises as the other sets. Antares and the surrounding stars also represented a scorpion in the mythology of the Maya and several other cultures. But others saw Antares differently. In China, it was the “fire star” – a description of its color. It and a couple of nearby stars represented the heart of a dragon. And in Hawaii, Antares was part of a fishhook used by the god Maui. The star itself is worthy of its reputation. It’s a dozen or more times heavier than the Sun, hundreds of times wider, and tens of thousands of times brighter – a supergiant star with some supergiant stories. Antares is just a skosh away from the Moon as they climb into good view tonight, by midnight. They’ll still be close as dawn twilight erases the scorpion’s mighty heart from view. Script by Damond Benningfield

    2 分钟
  3. 4天前

    Degenerate Future

    The Sun faces a “degenerate” future. That’s not a value judgment – it’s physics. When the Sun can no longer produce nuclear reactions, its core will collapse. How far it collapses is limited by a type of pressure exerted by its atoms – degeneracy pressure. Today, the Sun is “fusing” atoms of hydrogen to make helium. When the hydrogen is gone, it’ll fuse the helium to make carbon and oxygen. But the Sun isn’t massive enough to extend that process, so its nuclear furnace will be extinguished. Fusion releases energy, which balances the pull of gravity. That keeps the Sun puffed up. Right now, it’s big enough to hold a million Earths. When fusion stops, gravity will win out. The core will shrink to the size of Earth itself. But it’ll still be about half as heavy as the present-day Sun. So a chunk the size of a sugar cube would weigh a ton. The dead core won’t shrink beyond that. That’s because the electrons in the core will exert their own pressure – degeneracy pressure. They can be squeezed only so much before they run out of “elbow room” and halt the collapse. That will leave a white dwarf – a dead cosmic cinder – to cool and fade over the eons. The galaxy is littered with white dwarfs, but none of them is bright enough to see with the eye alone. The closest one is a companion of Sirius, the brightest star in the night sky, which is low in the southwest as night falls – a star that faces its own “degenerate” future. Script by Damond Benningfield

    2 分钟
  4. 6天前

    Desirable Stars

    The stars are quite literally desirable. That’s because the roots that make up the word desirable mean “to long for a star, heavenly body, or constellation.” Astronomy has a rich vocabulary: star, planet, galaxy, and many other words. Many of them also have non-astronomical meanings. A “galaxy of stars,” for example, might refer to an auditorium full of actors – though how many of them can be considered “stars” is a matter of opinion. Some words with heavenly connections seem obvious. “Lunatic” refers to the Moon. It comes from an ancient belief that the Moon’s influence could make people behave strangely. And “jovial” – to be full of good cheer – means “of Jupiter;” in ancient astrology, the planet was thought to exert a happy influence. Other words have more surprising connections to the stars. Consider “consider.” Its roots mean “to observe the stars.” “Sider” is from a Latin word that means “star, heavenly body, or constellation.” In fact, many words with some version of the root have a link to the stars – including desire. Disaster also comes from ancient astrology. It meant an unfavorable position for a star or planet. “Aster” was a Latin word for star. The word “influence” appeared in the 14th century. Dictionaries say it meant “streaming ethereal power from the stars when in certain positions, acting upon the character or destiny of men” – a good description of modern-day “influencers.” Script by Damond Benningfield

    2 分钟
  5. 4月29日

    Moon and Spica

    To the eye alone, Spica is one of the 15 brightest stars in the night sky. And it really is brilliant. At visible wavelengths, it’s about 2,000 times brighter than the Sun. It looks white with a hint of blue. When you look at Spica with special instruments, though, it’s even more impressive. It consists of two stars, not one. Both are much bigger and heavier than the Sun. And when you add up all wavelengths of light, they shine about 20 thousand times brighter than the Sun. Most of that energy is in the ultraviolet – wavelengths that are too short for the human eye. Spica’s two stars produce so much of it because their surfaces are tens of thousands of degrees hotter than the Sun’s. In fact, the type of energy a star emits depends almost entirely on its surface temperature. And so does the star’s color. To the eye alone, the hottest stars look blue. But they emit huge amounts of ultraviolet. The coolest stars look orange or red. They emit huge amounts of infrared light – wavelengths that are too long for the human eye. Stars in the middle are white or yellow. They emit most of their light at visible wavelengths. So with a star like the Sun, we see most of the energy it produces – light that’s just right for the human eye. Spica is quite close to the Moon as darkness falls this evening. The Moon will slide away from the star during the night, but they’ll still be close as they set, around dawn. Script by Damond Benningfield

    2 分钟
  6. 4月28日

    Venus and Aldebaran

    Aldebaran is like a reverse time capsule. Instead of preserving mementos from the past, the star shows us what we can expect in the distant future – the far, far distant future. It’s in a phase of life that the Sun will pass through in several billion years. Aldebaran marks the eye of Taurus, the bull. It’s low in the western sky as evening twilight fades. It’s a little to the left of Venus, the brilliant “evening star.” The Sun is in the prime phase of life. It’s steadily “fusing” the hydrogen atoms in its core to make helium. That produces the energy that makes our star shine. Aldebaran has already completed that phase. Its core has converted the hydrogen to helium. Now, the star is fusing the hydrogen in a thin layer around the core. This layer is especially hot. Its radiation pushes outward on the surrounding layers of gas. That’s caused Aldebaran to swell to about 45 times the Sun’s diameter. And that’s made the star more than 400 times brighter than the Sun. Over many millions of years, Aldebaran will use up that shell of hydrogen. Nuclear fusion will then fire up in the helium core, briefly making the star even bigger and brighter. After that, fusion in the core will begin to shut down. Aldebaran’s outer layers will blow away, briefly forming a colorful bubble. As the bubble dissipates, only the star’s now-dead core will remain – a final memento of a once impressive star. Script by Damond Benningfield

    2 分钟

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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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