StarDate

If you don’t like winter but you live in the northern hemisphere, then give a little thanks to the laws of orbital mechanics. Because of Earth’s lopsided path around the Sun, winter is the shortest season north of the equator. Earth’s orbit around the Sun isn’t a perfect circle. Instead, it’s an ellipse. It looks like a flattened circle, with the Sun slightly away from the center. Because of that shape, our distance to the Sun changes. And that’s where the laws of orbital motion come into play. Johannes Kepler devised those laws more than four centuries ago. One of them says that if you draw a line from the center of the Sun to the center of a planet, as the planet orbits the Sun that line will sweep out equal areas over equal periods of time. To do that, a planet must move fastest when it’s closest to the Sun, and slowest when it’s farthest from the Sun. Earth is closest to the Sun in early January – the start of winter – and farthest at the start of summer, in July. So Earth moves around the Sun in a hurry during northern winter, making the season shorter. This winter, for example, starts at 9:03 a.m. Central Time tomorrow. That’s the moment of the December solstice, when the Sun stands farthest south for the year. The season ends 89 days later. By comparison, this past summer lasted almost 93 days – a longer season thanks to the science of orbits. More about the solstice tomorrow. Script by Damond Benningfield

The “she-goat” is a lot more than it seems. What looks like a single brilliant star is actually two sparklers. Both of them are much bigger, heavier, and brighter than the Sun. Capella is the brightest star of Auriga, the charioteer. Its name comes from a Latin phrase that means the she-goat. It’s 43 light-years away – just down the block by astronomical standards. Both stars of Capella are about two and a half times as massive as the Sun. And both are more than 70 times brighter than the Sun. But the stars are quite close together – less than the distance from Earth to the Sun. So we can’t see them as individual points of light, even with the biggest telescopes. Astronomers discovered Capella’s dual nature with a technique called spectroscopy. It breaks a star’s light into its individual wavelengths. The spectrum of Capella shows two patterns of light. The patterns move back and forth as the stars orbit each other. The patterns reveal details about both stars – their surface temperature, composition, and more. From that and other details, we know that both stars have moved beyond the prime phase of life. Now, they’re in the giant phase. Both stars have puffed up to about 10 times the diameter of the Sun – two big, brilliant stars for the she-goat. Capella is a third of the way up the northeastern sky at nightfall. It’s one of the brightest stars in the entire night sky, so you can’t miss it. Script by Damond Benningfield

The tales that describe many of the ancient constellations can be romantic, tragic, heroic, or majestic. Some, on the other hand, are just weird. An example is Auriga. The constellation is low in the eastern sky at nightfall, and climbs high across the sky later on. It’s marked by a pentagon of stars. It’s easy to pick out thanks to the brightest member of that figure, Capella – one of the brighter stars in the entire night sky. Although Auriga is described as a charioteer, the character usually isn’t depicted with a chariot. But he is shown with a goat and her two kids on his shoulder. There are several versions of his story. In one, he was an early king of Athens. He was raised by the goddess Athena. Among other things, she taught him how to tame horses. He was so good at it that he became the first person to harness four horses to a chariot, like the chariot that carried the Sun across the sky. Zeus, the king of the gods, was so impressed that he placed the charioteer in the stars. The goat is represented by Capella. It isn’t a part of any of the legends of Auriga from Greek or Roman mythology. It may represent the goat that suckled the infant Zeus, who placed her and her children in the sky in gratitude. The goat and kids may once have formed their own small constellation. Today, though, they ride on the shoulder of the charioteer – who rides on nothing at all. More about the charioteer tomorrow. Script by Damond Benningfield

At the cusp of the 20th century, it seemed like contact with another world was just a matter of time. In fact, the French Academy of Sciences announced a prize for such a feat 125 years ago today. The winner would receive 100,000 francs. There was only one catch: Mars didn’t count. The prize was established by Clara Guzman in honor of her son. He was a follower of astronomer Camille Flammarion, who wrote extensively – and fancifully – about the Red Planet. Guzman excluded Mars from the competition because it seemed just too easy. Percival Lowell had popularized the idea that Mars was crisscrossed by canals – built by Martians to bring water from the poles to the planet’s deserts. Inventor Nicola Tesla had reported hearing possible radio signals from Mars. And many others thought that vast dark areas on Mars were covered with vegetation. Many schemes were proposed to contact the Martians. One suggested creating giant geometric shapes in Siberia. Another suggested digging the shapes into the Sahara Desert, filling them with kerosene, and setting them on fire. None of the schemes ever materialized. And no one ever claimed the prize for contacting another world. So the French academy decided to award the prize for making physical contact. In 1969, it awarded the Guzman Prize to Apollo 11 astronauts Neil Armstrong, Buzz Aldrin, and Michael Collins – the first men to set foot on another world. Script by Damond Benningfield

The planet Mercury is shrinking. It’s contracted by several miles since its birth. And it’s continuing to get smaller even now. Mercury is the closest planet to the Sun. It’s also the smallest major planet in the solar system – a little more than 3,000 miles in diameter – about the width of the 48 states. It has a core of iron and nickel, surrounded by dense layers of rock. And it’s topped by a thin crust. The surface of the planet is marked by lots of impressive cliffs. The biggest is more than 600 miles long and about two miles high. They formed as Mercury lost heat from its interior. As the planet cooled, it shrank. Estimates of how much it’s contracted have ranged from about a mile to about nine miles. A recent study narrowed the range a little bit. It measured the most dramatic features, then scaled that to the surface of the entire planet. The result suggests that Mercury has shrunk by about three to five miles as a result of its cooling. And when you add in some other causes, the total contraction is about four to seven miles. And Mercury is still getting smaller today. This incredible shrinking planet is quite low in the southeast in the dawn twilight for the next few days. It looks like a bright star, but you need a clear horizon to spot it. And because of the viewing angle, it’s easier to spot from more southern latitudes. Tomorrow, the Moon stands to its right or upper right. Script by Damond Benningfield

Here’s what we know for sure about the planet K2-18b. It’s about 125 light-years away. It’s bigger and heavier than Earth. It orbits a cool, faint star once every 33 days. It receives about the same amount of energy from its star as Earth gets from the Sun. And it has an atmosphere. After that, things get muddled. Astronomers aren’t sure about the structure of the planet or the make-up of its atmosphere. And ideas about whether it might be habitable are all over the place. The confusion highlights the challenges of studying planets in other star systems. K2-18b passes in front of its star on every orbit. And as it does so, the chemical “fingerprints” of its atmosphere are added to the starlight. Substracting the starlight provides a profile of the atmosphere. But the profile is hard to read. Many of the fingerprints are subtle, and can be produced by different compounds. Earlier this year, a team announced the discovery of compounds in the atmosphere that could be produced by microscopic life. Follow-up studies by other groups contradicted that finding. But the original study team has stuck by its conclusions. So it’ll take a lot more work to know for sure what’s going on at K2-18b. The K2-18 system is in Leo, which climbs into good view after midnight. K2-18 is to the right of Denebola, the star that marks the lion’s tail. But it’s too faint to see without a telescope. Script by Damond Benningfield

For stars that are similar to the Sun, the end comes in stages. And each stage is triggered by changes in the star’s core. One star that’s going through those changes is Diphda, the brightest star of Cetus, the sea monster. The star is several hundred million years old – billions of years younger than the Sun. For most of its life, it “fused” hydrogen atoms in its core to make helium. When the hydrogen was gone, it began fusing hydrogen in a shell around the core. That made the star puff up, so it was classified as a red giant. Now, it’s finished off the shell, so it’s fusing the helium in the core to make carbon and oxygen. This phase is generally lumped into the red-giant category. Technically, though, it has its own name: the red clump. In a hundred million years or so, Diphda will have used up all the helium. The star isn’t massive enough to fuse the carbon and oxygen to make heavier elements. Without that energy, the core will collapse to about the size of Earth. It’ll be extremely hot, though, so it’ll blow away Diphda’s outer layers. For a while, the star will enter one more phase: a planetary nebula – a colorful cloud of gas and dust. When the cloud disperses, only the dead core will remain: a white dwarf – the hot but tiny remnant of a star. Cetus spreads across the southeastern quadrant of the sky at nightfall. Diphda is near its lower right corner, roughly a third of the way up the sky. Script by Damond Benningfield

People collect all kinds of things, from baseball cards to Persian rugs. Over the past 40 years, some NASA aircraft have collected dust – grains of dust from beyond Earth. Many of the collection efforts have taken place during meteor showers. That’s included the Geminid shower, which is at its peak tonight. A meteor shower takes place when Earth flies through a trail of particles that were shed by a comet or asteroid. Many of the particles burn up in the upper atmosphere, creating the streaks of light known as meteors. But many more grains are too small to burn up. They float down through the atmosphere. Some of them stop at a height of about 10 miles. And that’s where the research aircraft head. Once there, they open up small boxes that catch whatever is drifting along – pollen grains, parts of bugs, bits of volcanic ash, and even exhaust from rocket engines. Analysis reveals whether the captured particles are from Earth or from outside. The cosmic particles can then be tied to the meteor shower that was under way. And that can tell scientists about the shower’s parent body – a sample-return mission that never leaves Earth. The Geminids are in good view tonight. The meteors are visible from mid-evening on. At its best, the shower might produce a hundred or so meteors per hour. And you don’t need to look in a particular direction to see them – just look up and wait for the fireworks. Script by Damond Benningfield

A couple of thousand years ago, a large asteroid or comet might have been blasted apart. And we’re still seeing the fireworks from its destruction – as the Geminid meteor shower, which will reach its peak tomorrow night. Most meteor showers flare to life when Earth passes through the orbital path of a comet. The comet sheds bits of rock and dirt, which spread out along its orbit. As Earth flies through this trail of debris, the solid grains ram into the atmosphere, forming the glowing streaks known as meteors. But the Geminids are a bit odd. For one thing, their parent body – 3200 Phaethon – appears to be an asteroid or a “dead” comet, not an active comet. For another, the meteor stream contains way more material than we’d expect to see from a body the size of Phaethon. A couple of years ago, scientists came up with a possible explanation. They used observations by a Sun-orbiting spacecraft that passed through the meteor stream. They then used computer models to calculate a possible cause for the stream. They concluded that a larger body could have been destroyed. That produced Phaethon and a couple of other large remnants. But it also produced a giant cloud of dust and pebbles. So while some of the material that makes up the Geminids comes from Phaethon, a lot of it also comes from that cloud – shrapnel that makes fireworks in Earth’s night sky. More about the Geminids tomorrow. Script by Damond Benningfield

The Sun isn’t easy to influence. It’s more than a thousand times the mass of Jupiter, the solar system’s largest planet, and more than 330,000 times the mass of Earth. Even so, a recent study says the planets might influence our star’s magnetic cycle – perhaps making conditions more comfortable for life. The Sun goes through many cycles of magnetic activity. The best known lasts an average of 11 years. At the cycle’s peak, the Sun is much more active than average. It pelts Earth and the other planets with higher levels of radiation and charged particles. That can wreak havoc with everything from satellites to blood pressure. Another cycle lasts an average of less than two years. It produces “mini” peaks and valleys in the 11-year cycle. And it lines up well with the longer cycle. In the recent study, researchers from Germany compared these cycles to the orbits of the planets. They found that the peaks and valleys of the shorter cycle correspond to some planetary alignments. One was a lineup of Earth, Jupiter, and Venus. The other was an alignment of Jupiter and Saturn. The researchers said the planets may help control the solar cycles. The planets might even tamp down the Sun’s activity, which is weaker than that of many Sun-like stars. Less activity means that Earth gets bombarded by less of the nasty stuff – making our planet a much more comfortable home for life. Tomorrow: cosmic shrapnel. Script by Damond Benningfield

Storms on the Sun can cause all kinds of problems. They can knock out satellites and black out power grids. They can interfere with GPS and disrupt some radio broadcasts. They can even have an impact on human health. Solar storms happen when the Sun’s magnetic field gets tangled up. Lines of magnetic force can snap, then reconnect. That produces outbursts of radiation and charged particles. When the particles hit Earth, they’re funneled toward the surface by our planet’s own magnetic field. And that’s what causes the problems. Among the health concerns, particles and radiation can penetrate deeper into the atmosphere around the magnetic poles. That zaps anyone who’s flying at high altitudes in those regions. It’s not a fatal dose, but it’s enough to cause concerns. So airlines divert flights to avoid exposing passengers and crew. There’s also evidence that these bouts of “space weather” can boost people’s blood pressure. In one study, researchers in China looked at half a million blood pressure readings taken over six years. And they found a definite jump around the time of solar storms – especially among women and those with hypertension. An American team found similar results among older men. There’s no consensus about how space weather might cause blood pressure to spike. For now, all we know is that stormy skies on the Sun can cause lots of problems for the people on Earth. Script by Damond Benningfield

The Moon and the heart of the lion just miss each other tonight – at least as seen from the United States. As they climb into good view, after midnight, the Moon and the star Regulus will be separated by just a skosh. The farther north and east your location, the closer together they’ll appear. From some spots, they’ll be almost touching. And from much of Canada across to northern Norway they will touch – the Moon will occult the star. It’ll pass directly in front of Regulus, blocking it from view. The Moon can occult Regulus because the star lies almost atop the ecliptic – the Sun’s path across the sky. The Moon stays close to the ecliptic as well, but it does move a few degrees to either side. As a result, occultations of Regulus come in groups. This one is part of a cycle of that began earlier this year and will continue through the end of next year. Each occultation is visible from a different part of Earth. In part, that’s because each one lasts only a few minutes to a few hours, so the Moon and Regulus are below the horizon as seen from much of the world. Also, the Moon is so close to us that there’s a big difference in the viewing angle across the globe – up to two degrees – four times the width of the Moon itself. From any specific location, sometimes the angle is just right, but more often it’s a little off – providing a beautiful close encounter between the Moon and the heart of the lion. Script by Damond Benningfield

A couple of years ago, a space telescope discovered something odd about NGC 6505. The galaxy is encircled by a ring. It isn’t part of the galaxy itself. Instead, it’s an image of a background galaxy – one that’s billions of light-years farther. Einstein Rings are named for Albert Einstein because they were predicted by his theory of gravity. The gravity of a foreground object acts as a lens – it bends and magnifies the light of a background object. On small scales, gravitational lenses have revealed everything from black holes to rogue planets. Galaxies are much bigger and heavier, so they produce more dramatic lenses. Many of them create bright arcs. But when the alignment is just right, they can create a full circle. NGC 6505 is a good example. The galaxy is about twice the diameter of the Milky Way, and several times its mass. It’s about 600 million light-years away. The background galaxy is four billion light-years farther. The lensing effect has allowed astronomers to measure the amount of dark matter in the center of NGC 6505, as well as details about its stars – discoveries made possible by its beautiful ring. NGC 6505 is enwrapped in the coils of Draco, the dragon. The galaxy is more than a third of the way up the northwestern sky at nightfall. It’s visible through a small telescope. But you need a big telescope and a long exposure to make out its ring. Script by Damond Benningfield

The Moon is a “dead” world. It trembles with a few small moonquakes, and there may be occasional “burps” of gas. But for the most part, not much happens inside it. That’s definitely not the case for one of the moons of the giant planet Jupiter. Io is the most volcanically active world in the solar system. It’s covered by hundreds of volcanoes and pools of hot lava. Some of the volcanoes are larger than anything on Earth, and the lava is much hotter. The volcanoes can send gas and ash hundreds of miles high. Some of this material escapes Io completely – about one ton every second. It forms a wide “doughnut” around Jupiter. The activity is powered by a gravitational tug-of-war between Jupiter and some of its other big moons. They pull on Io in different directions. That heats Io’s interior, melting some of its rocks. A couple of recent studies found that Io has been at least this active since it was born. That suggests that Io and the other big moons have been locked into their current configuration since shortly after the birth of Jupiter itself. If that’s the case, then Io has been caught in a terrific tug-of-war for four and a half billion years. Jupiter rises above our moon this evening. The planet looks like a brilliant star – only the Moon and Venus outshine it. But you need binoculars to pick out Io and the planet’s other big moons. Tomorrow: gravitational “rings” around a galaxy. Script by Damond Benningfield

The Moon forms a beautiful grouping with the planet Jupiter and the twins of Gemini tonight. Jupiter looks like a brilliant star. It’s below the Moon as they climb into view, by about 8:30. Castor, the fainter of Gemini’s twins, is to the left of the Moon. And Pollux, the brighter twin, is to the lower left. The grouping is even tighter at first light tomorrow. The Moon circles through Gemini roughly once a month – the time it takes to complete one full turn through the background of stars. If you made a movie of those passages over the years, the Moon would look like a car that can’t stay in the same lane. That’s because the Moon’s orbit around Earth is tilted a bit compared to the ecliptic – the Sun’s path across the sky. So the Moon moves back and forth across the ecliptic during its month-long cycle. It moves from about five degrees north of it, to about five degrees south. The Moon’s position on the ecliptic relative to an individual constellation doesn’t change much from month to month. Instead, it takes years to see much of a difference. In the case of Gemini, that means that every few years the Moon comes especially close to Pollux. But then it moves away, and eventually leaves a big gap – up to the width of your fist held at arm’s length. But that won’t happen again until the early 2030s, as the Moon weaves into another lane. More about the Moon and Jupiter tomorrow. Script by Damond Benningfield

For radio astronomers, there’s some good news and some bad news. On the good side, a pilot project with SpaceX has devised a way to reduce the radio interference produced by satellites. On the bad side, the satellites can produce accidental interference. Radio telescopes tell us things about the universe that we can’t get any other way. But the telescopes are extremely sensitive. Transmissions from an orbiting satellite are like bright headlights – they overpower the subtle signals of astronomical objects. There are more than 15,000 satellites in orbit today – a five-fold increase in just six years. And the total could balloon to a hundred thousand by the next decade. Astronomers worked with SpaceX to reduce interference from its Starlink satellites. The groups combined the observing schedule of a telescope with the Starlink control system. Satellites passing over the telescope were instructed to turn away – aiming the headlights in a different direction. And there are plans to extend the scheme to other telescopes. On the other hand, a recent study found that tiny radio signals emitted by a satellite’s electronics can also be a problem. Scientists looked at 76 million radio images made by a telescope in Australia. They found that Starlink satellites interfered with up to 30 percent of the pictures. So future satellites may need extra shielding to keep them from blinding astronomy’s radio eyes. Script by Damond Benningfield

Most of the stars are so small and far away that they’re nothing more than pinpoints even in the largest telescopes. That makes it impossible to measure the size of a star. But astronomers can measure the sizes of some stars – not with a giant telescope, but with a collection of smaller ones. The technique is called interferometry. It links up several telescopes. The combo provides an especially sharp view of the heavens. If the telescopes are, say, 300 feet apart, then the combined view is as clear as that of a single telescope 300 feet in diameter. The array’s view isn’t as deep as that of a giant telescope, only as sharp. Interferometers have allowed astronomers to measure the apparent sizes of hundreds of stars. Combining that with a star’s distance provides its true size. One example is Elnath, the second-brightest star of Taurus. It’s about 134 light-years away. It’s five times the mass of the Sun. So even though it’s much younger than the Sun, it’s already passed through the prime phase of life. That’s caused it to puff up – to almost five times the Sun’s diameter. At that size, it shines more than 800 times brighter than the Sun – a big beacon for the bull. Elnath is close to the lower left of the Moon this evening. The Moon will move toward the star during the night. They’ll be closest at dawn. The gap will be smaller for skywatchers on the West Coast, and smallest for those in Alaska and Hawaii. Script by Damond Benningfield

[3, 2, 1, ignition, and liftoff of SOHO and the Atlas vehicle on an international mission of solar physics.] Generally speaking, staring at the Sun non-stop for decades is a bad idea. But a spacecraft launched 30 years ago this week has done just that. It’s told us about the Sun’s interior, its surface, and its extended outer atmosphere. That’s helped scientists develop better forecasts of space weather – interactions between Sun and Earth that can have a big effect on our technology. The craft is called SOHO – Solar and Heliospheric Observatory. It was launched into an orbit around a point in space where the gravity of Earth and the Sun are balanced. From there, its view of the Sun is never blocked. SOHO watches the Sun in many different ways. It keeps a close eye on the Sun’s magnetic field, which produces outbursts of energy and particles that can have an impact on Earth. That’s revealed shockwaves and “tornadoes” rippling across the Sun’s surface. It’s also revealed the source of the solar wind – a steady flow of charged particles that blows through the solar system. Some of SOHO’s observations block out the Sun itself, showing the space around the Sun. That’s allowed SOHO to discover more than 5,000 comets as they passed close to the Sun – many of which didn’t survive. SOHO’s mission is scheduled to end soon – closing this long-working eye on the Sun. Script by Damond Benningfield

Scientists have been searching for dark matter for decades. They haven’t found it – every experiment they’ve devised has come up empty. But they haven’t given up. Among other ideas, they’re thinking about ways to use moons, planets, and stars as detectors. Dark matter appears to make up about 85 percent of all the matter in the universe. We know it’s there because its gravity pulls on the visible stars and galaxies around it. Dark matter may consist of a type of particle that almost never interacts with normal matter. But it should interact just enough to reveal its nature. Experiments here on Earth haven’t seen any such interactions. So some scientists recommend using astronomical objects instead of lab experiments. Blobs of dark matter might enfold a binary star system. The dark matter’s gravity could pull the two stars away from each other. And dark matter might clump together to make a special kind of star. Both of those might be detectable with current telescopes. Smaller blobs might slam into an icy moon, creating a special kind of crater. Such craters could be visible on Ganymede, the largest moon of Jupiter. Two missions on their way to Jupiter might be able to see them. And dark matter might fall into the center of a planet and hang around. If enough builds up, it could heat the planet’s interior. So by studying many planets in other star systems, we might see some that are unusually warm – heated up by encounters with dark matter. Script by Damond Benningfield

Things are heating up for a planet that orbits the brightest star of Aries. The star is expanding to become a giant, so it’s pumping more energy into space. That will make temperatures extremely uncomfortable on the planet. Hamal is at the end of its life. It’s converted the hydrogen in its core to helium. Now, it’s getting ready to fuse the helium to make other elements. That’s made the core hotter. And that’s caused the star’s outer layers to puff up – to more than a dozen times the diameter of the Sun. So Hamal is about 75 times brighter than the Sun. Hamal has one known possible planet. It’s heavier than Jupiter, the giant of our own solar system. On average, the planet is about as far from Hamal as Earth is from the Sun – much closer in than Jupiter is. So every square foot of the planet’s surface receives dozens of times more energy than the same area on Jupiter does. If the planet is a ball of gas like Jupiter, then the extra heat is causing its atmosphere to puff up – and causing a lot of it to stream away into space. Over the next few million years, the planet will get even hotter, because Hamal will get even bigger. The extra energy may erode the planet’s atmosphere completely. On the other hand, the planet may spiral into the star. Either way, things are going to get much hotter for Hamal’s only known planet. Look for Hamal in the east at nightfall, well to the left of the Moon. Script by Damond Benningfield