『StarDate』のカバーアート

StarDate

StarDate

著者: Billy Henry
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10月19日まで。※適用条件あり
StarDate, the longest-running national radio science feature in the U.S., tells listeners what to look for in the night sky.© 2022 The University of Texas McDonald Observatory 博物学 天文学 天文学・宇宙科学 日次 科学 自然・生態学
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  • Moon and Antares
    2026/10/14

    Antares, the bright star at the heart of Scorpius, huddles quite close to the Moon early this evening. They set not long after the sky gets dark, so there’s not a lot of time to look for them.

    The Moon is a thin crescent now, so it’s night across most of the lunar disk. But on the bright sliver that’s in daylight, you can still make out some of the dark lunar “seas” – vast plains of volcanic rock. They formed long ago, when giant asteroids slammed into the Moon. Molten rock bubbled up from below, then cooled and hardened.

    A recent study found evidence of an especially big impact three-and-a-half billion years ago. The hit would have been powerful enough to melt the surface across a wide area.

    Researchers discovered the evidence in a meteorite known as Northwest Africa 12593. It was found in Mali, in 2017. It contained some tiny crystals that form only under extreme heat. The chemistry of the meteorite suggested the impact happened three-and-a-half billion years ago.

    A later impact shattered the lava plain, jumbling up the rocks. And a third impact blasted some of the fragments into space, including the one that fell to Earth. The initial impact happened at about the time of similar events on Earth and the asteroid Vesta. That suggests that the inner solar system was littered with many giant space rocks at the time – cosmic “missiles” that sometimes smashed into Earth and the other large worlds.

    More tomorrow.

    Script by Damond Benningfield

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    2 分
  • Quiet Monster
    2026/10/08

    A quiet monster lurks in the heart of M31, the Andromeda Galaxy. Known as M31-star, it’s a black hole a hundred million times the mass of the Sun, and 25 times heavier than the black hole at the heart of the Milky Way.

    Every large galaxy probably has a supermassive black hole. And many of them are quite bright.

    The black hole itself is completely black – it swallows up all the matter and energy that falls into it, and nothing can come back out.

    But the black hole’s gravity pulls in huge amounts of gas and dust, along with an occasional asteroid, star, or other large object. This debris forms a disk around the black hole. As material in the disk spirals closer to the black hole it gets extremely hot, so it shines brightly.

    But M31-star is one of the quietest of all supermassive black holes – its disk produces very little energy.

    That tells us that the black hole is not actively “feeding” – not much debris is falling into it. A distant ring of gas and dust encircles the black hole, with filaments of material spiraling into the disk. But the “feeding” rate is low, so M31-star remains quiet – a dark monster in the heart of M31.

    Under dark skies, the Andromeda Galaxy is visible to the naked eye. It looks like a faint smudge of light that’s wider than the Moon. Right now, it’s about a third of the way up in the east-northeast at nightfall, and climbs high overhead later on.

    Script by Damond Benningfield

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    2 分
  • Caroline’s Rose
    2026/10/09

    Cassiopeia is an easy constellation to pick out. The stars of the queen form a prominent letter M or W, which is visible even through moderate light pollution. And under dark skies, binoculars reveal several star clusters around that pattern, all immersed in the glow of the Milky Way.

    One of the highlights is NGC 7789. It was discovered in 1783 by Caroline Herschel – the first woman to be paid for her work as an astronomer. Through a telescope, the contours of the cluster and nearby clouds of dust resemble a rose. So NGC 7789 also is known as Caroline’s Rose.

    The cluster is about 6800 light-years away, in the opposite direction from the center of the galaxy. And it’s packed with stars. It has 1300 confirmed members, with an estimated total of 3,000 stars or more.

    The cluster’s age has been tough to pin down. A recent study says it’s one-and-a-quarter billion years old. Previous estimates are a little higher. Regardless of the exact age, the cluster has made several orbits around the center of the galaxy. By the time many other clusters have made that many orbits, they’ve been pulled apart by the gravity of the rest of the galaxy. The stars survive, but they head their separate ways. Caroline’s Rose is in the northeast at nightfall, just above Cassiopeia’s outline. It climbs high across the north during the night.

    Script by Damond Benningfield

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    2 分
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