10 épisodes

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

StarDate Billy Henry

    • Sciences

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

    Hercules Cluster

    Hercules Cluster

    In our region of the Milky Way Galaxy, the stars are a long way apart. The Sun’s nearest neighbor is more than four light-years away — 25 trillion miles. In the core of a globular cluster, though, the stars are packed hundreds of times more densely. That means the stars are only a few light-months apart, or even light-weeks — much closer than in our own neighborhood.



    One of the most prominent globular clusters is in Hercules, the strongman. M13 — the Hercules Cluster — is perhaps 25,000 light-years away. It contains several hundred thousand stars.



    M13 and the other globular clusters are thought to be the oldest inhabitants of the Milky Way. So most of the stars in the cluster are more than 10 billion years old — more than twice the age of the Sun.



    Such stars are fainter, redder, and less massive than the Sun. From a planet near the cluster’s middle, you’d see a whole bunch of stars in the night sky, and almost all of them would be yellow, orange, or red — remnants of the early galaxy.



    M13 is low in the northeast at nightfall. It’s along the line that connects the top two stars in the “Keystone” — a lopsided square of stars that outlines the strongman’s torso. Under clear, dark skies, the cluster looks like a dim fuzzball. It’s easier to see if you look out of the corner of your eye. It’s an easy target for binoculars — the glow of an ancient family of stars.



    Script by Damond Benningfield

    • 2 min
    Hercules

    Hercules

    The geography of the sky owes a lot to Claudius Ptolemy. He was a Greek astronomer who lived and worked in Alexandria, the capital of Greek-controlled Egypt.



    Almost 1900 years ago, Ptolemy published one of the most important astronomical works in history. Known as the Almagest, it contained Ptolemy’s models of the motions of the Sun, Moon, and planets, and much more. One of its most important features was a catalog of stars and constellations. It listed 48 constellations visible from the northern hemisphere, most of which had been around for thousands of years. And, thanks to Ptolemy, they’re still with us today.



    The list includes Hercules, the strongman. The constellation is in the east and northeast at nightfall, and swings high overhead during the night.



    “Hercules” is the Roman version of Heracles, a son of Zeus, the king of the Greek gods of Olympus. His mother was not Zeus’s wife, Hera, and Hera wasn’t happy about the situation. She tried to kill the baby, but he survived. She then set about making his life miserable.



    Hera drove the adult Heracles mad, causing him to kill his family. To atone for his crimes, he was given 12 labors to complete — tests of strength, courage, and skill. Eventually, Hera relented, and allowed Heracles to join the gods on Mount Olympus — and to be placed among the stars — one of the constellations preserved by Claudius Ptolemy.



    We’ll have more about Hercules tomorrow.



    Script by Damond Benningfield

    • 2 min
    Leo Triplet

    Leo Triplet

    Most of the “star pictures” in the night sky look nothing like their namesakes. But one beautiful exception lunges across the southwestern sky on May evenings: Leo, the lion. It’s high in the sky at nightfall.



    Leo consists of two patterns of stars that the brain puts together to make a lion. A backward question mark represents the head and mane. And a triangle of stars to the lower left forms the lion’s hindquarters and tail.



    Leo is best known for its bright stars — especially Regulus, its brilliant heart. But the constellation also contains quite a few bright galaxies. Leading the list are three galaxies that form the Leo Triplet: M65, M66, and NGC 3628.



    NGC 3628 is the most interesting of the three. Like our own Milky Way, it’s a spiral — a pinwheel that spans at least a hundred thousand light-years. We see it edge-on, so it looks like a streak of light with lines of dark dust running down the middle.



    Close encounters with the other galaxies have pumped up NGC 3628. They’ve triggered the birth of millions of new stars near the galaxy’s core. And they’ve pulled out a tail of gas that spans a quarter of a million light-years — enough gas to make half a billion stars as massive as the Sun. In fact, the tail has given birth to millions of stars already.



    The Leo Triplet is just one of the wonders in one of the night sky’s most easily recognizable constellations: the lion.



    Script by Damond Benningfield

    • 2 min
    Moon and Mercury

    Moon and Mercury

    Over the centuries, no planet has been as frustrating to study as Mercury. The Sun’s closest planet never moves far from the Sun in our sky. So when astronomers pointed telescopes at Mercury, it was almost always screened by twilight and a thick layer of Earth’s atmosphere. So most of what we know about Mercury has come from spacecraft that visited the planet.



    You can see the difficulty yourself the next few days. Mercury is quite low in the east not long before sunrise. It’s almost at its farthest point from the Sun, and it looks like a fairly bright star. But at that low altitude, its light has to pass through a thick layer of air, which blurs the view. The glow of twilight makes the view even murkier.



    Without the ability to see surface features, it was hard to nail down the length of Mercury’s day. The planet always shows the same face when it’s closest to Earth. So it looked like Mercury was locked so that the same hemisphere always faced the Sun, just as the same side of the Moon always faces Earth.



    But that’s not right. Radio telescopes have showed that Mercury makes three turns on its axis for every two orbits around the Sun. That means a “day” on Mercury — the time from one noon to the next — lasts 176 Earth days — long days and nights for the Sun’s closest planet.



    Mercury appears near the Moon the next couple of mornings. It’s to the lower left of the Moon tomorrow, and closer to the right on Monday.



    Script by Damond Benningfield

    • 2 min
    Moon and Planets

    Moon and Planets

    The atmosphere of Mars is quite different from Earth’s. It’s colder, thinner, and it’s made mainly of carbon dioxide. In one way, though, the skies of the two planets are similar: both of them have clouds. And for the most part, the clouds themselves are alike as well.



    Because Mars is so cold, the clouds are made entirely of ice — frozen water or carbon dioxide. There’s not much water in the Martian atmosphere, so the clouds are thin. And they’re usually much higher than even the highest clouds of Earth.



    But Mars also has some clouds that are a bit different from those on Earth. That includes “dots” and some long, skinny ribbons.



    An orbiting spacecraft has seen the dots in a specific region of Mars, south of the equator. The clouds are almost perfectly round. They’re up to 60 miles in diameter, a few miles thick, and they top out at altitudes of 30 to 50 miles. Some are seen at dawn, while others are seen in clumps in the dawn or evening twilight. The clouds could form as the atmosphere interacts with some odd spots in the Martian magnetic field.



    The elongated clouds are seen in volcanic regions. The longest span about 1500 miles, and are up to a hundred miles wide. They may be sculpted by winds flowing over volcanic peaks — some odd clouds for the Red Planet.



    Mars stands close to the lower left of the Moon at dawn tomorrow. The planet Saturn is about the same distance to the upper right of the Moon.



    Script by Damond Benningfield

    • 2 min
    Moon and Saturn

    Moon and Saturn

    The solar system is pretty settled. The planets appear to be following orbits that have remained stable for billions of years. But in the early days, things might have been a lot more chaotic. According to one model, in fact, the giant planets Jupiter and Saturn might have moved much closer to the Sun before they moved back out again.



    The planets probably took shape from a disk of gas and dust around the Sun. Small bits of material stuck together to make bigger bits, all the way up to planets. But much of the material remained free. There was enough of it to exert both a drag and a pull on the giant planets.



    In this model, Jupiter — the Sun’s heaviest planet — was born at about two-thirds of its present distance from the Sun. It quickly moved inward, though, all the way to the orbit of Mars. Saturn — the second-most-massive planet — was dragged inward as well. Jupiter and Saturn thinned out the supply of gas and dust and the leftover planetary building blocks — either by scooping them up or kicking them away from the Sun. That changed the gravitational balance of the solar system. Jupiter and Saturn moved outward — settling into their current stable orbits around the Sun.



    Saturn is in the dawn sky now, and looks like a bright golden star. Unlike a star, though, it doesn’t twinkle — its light holds steady. Tomorrow, it will stand close to the left of the Moon. The Moon will pass between Saturn and Mars the next morning; more about that tomorrow.



    Script by Damond Benningfield

    • 2 min

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