StarDate

For skywatchers across the eastern United States, the planet Jupiter will vanish early tomorrow – hidden behind the crescent Moon. The rest of the country will see an impressively close encounter between the two bodies.

The vanishing act is an occultation – from a Latin word that means “to hide.” Over the centuries, astronomers used these events to learn more about the Jovian system. Precise timing of occultations helped astronomers understand the planet’s orbit, which helped them zero in on Jupiter’s distance. And it takes a few seconds for the planet to vanish and reappear. The exact timing, combined with Jupiter’s distance, helped refine its diameter.

Occultation studies also have included radio waves. Jupiter’s magnetic field sculpts a teardrop-shaped “bubble” around the planet. It also creates powerful radiation belts. Watching Jupiter vanish behind the Moon revealed the extent of both.

Occultations are less important to scientists than they once were – but they’re still fun to watch.

This one plays out before or during dawn. Jupiter looks like a brilliant star. From the eastern U.S., it’ll wink out before dawn, with Jupiter and the Moon quite low in the sky. From a little farther west, the occultation will be in progress as they rise, with Jupiter popping into view shortly thereafter. Those in the western states will have to settle for an especially close encounter between Jupiter and the Moon.

Script by Damond Benningfield

To borrow from “Alice in Wonderland,” the case for life on Mars keeps getting curiouser and curiouser. Two rovers have discovered organic compounds there – the chemical building blocks of life – in locations that are thousands of miles apart. And some recent looks at results from the Viking landers of the 1970s suggests they, too, might have found organics. So it’s possible that microbes might have inhabited Mars in the past – and might do so even today.

Some of the best evidence comes from the Perseverance rover. In 2024, it studied a formation known as Bright Angel – layers of sediment deposited at the bottom of a river perhaps three and a half billion years ago.

A rock named Cheyava Falls contained a lot of organics. And a study earlier this year confirmed the finding. The compounds could have been produced by microscopic life. But there are several other possible explanations, including chemical reactions in the rocks themselves.

Perseverance stored a sample of Cheyava Falls for return to Earth. Laboratory analysis could tell us for sure how the organics were formed. But NASA has nixed a planned sample-return mission. So we’re a long way from satisfying our curiosity about life on Mars.

Look for Mars quite near the Moon early tomorrow. It looks like a bright star. They’re especially close as they climb into good view, around 2:30 or 3.
We’ll talk about the Moon and another companion tomorrow.

Script by Damond Benningfield

The Moon will run a gauntlet of bright stars and planets the next few mornings, from the twins of Gemini to the heart of the lion. The twins are up first. Pollux and Castor will perch to the upper left of the Moon at dawn tomorrow. Pollux is the brighter of the two, and it’ll be closer to the Moon. On the following mornings, the Moon will slide past Mars, Jupiter, and Regulus.
These encounters are possible because all of these objects are near the ecliptic – the Sun’s path across the sky. The stars all maintain the same position relative to the ecliptic from month to month and year to year. Regulus, for example, is less than half a degree away from it – less than the width of a pencil held at arm’s length.
The planets, on the other hand, can shift from one side of the ecliptic to the other. That’s because their orbits around the Sun are tilted a bit.
The Moon’s orbit is tilted as well, by about five degrees. So the Moon can swing a little farther from the ecliptic. Tonight, it’s a few degrees north of it. By Wednesday, when it’s closest to Regulus, it’ll be just south of it.
Despite that wiggle room, the Moon passes close to each of these bright pinpoints during every month-long cycle of phases. And when the geometry is just right, it can even cover them up – which it will do to Jupiter on Tuesday. We’ll have more about that later in the week, and more about the Moon and Mars tomorrow.

Script by Damond Benningfield

Saturn is a “superior” planet. Among other things, it’s the second-largest and second-heaviest planet in the solar system. Technically, though, what makes it “superior” is its location. It’s the sixth planet from the Sun, so its orbit is outside Earth’s orbit.

Superior planets can line up opposite the Sun in our sky – a point known as opposition. And that’s what Saturn is doing now. It’ll reach that point early Sunday. So for a while, it’ll be in the sky all night, and shine brightest for the year. Only a few planets and stars will outshine it.

A planet looks especially bright at opposition for a couple of reasons. For one thing, it’s closest to Earth. Saturn, for example, will be about a hundred million miles closer than average.

Another reason is the viewing angle. At opposition, a planet is reflecting more sunlight directly toward Earth than at any other time. In effect, the planet is a more efficient “mirror.” We see the same effect with the Moon. A full Moon – which also is in a “superior” position – is about six times brighter than a half Moon. The change in the Moon’s brightness is complicated by other factors, but the principle is the same – a superior Moon puts in a superior show – just like the superior planet Saturn.

Saturn is low in the east at nightfall. It looks like a bright star. It climbs high across the south during the night, and is low in the west at dawn.

Script by Damond Benningfield

This isn’t a sound effect from a sci-fi movie. Instead, it’s the “voice” of the auroras on the planet Saturn – radio waves that have been shifted to wavelengths we can hear. They were recorded by the Cassini spacecraft as it closed in on Saturn two decades ago.

The radio waves are produced by the complex interplay between Saturn’s magnetic field and the solar wind – a steady flow of charged particles from the Sun.

Motions deep inside the planet generate the magnetic field, which is about as strong as Earth’s. But because Saturn is much bigger than Earth, its magnetic field is much bigger as well – it fills a huge volume of space.

The magnetic field forms a teardrop-shaped “bubble” around Saturn. That bubble deflects much of the solar wind. But some of the particles make it through. The lines of magnetic force guide some of them toward the magnetic poles. They spiral in, emitting radio waves as they do so. And when the particles hit the upper atmosphere, they create auroras – shimmering curtains powered by the Sun.

Saturn is putting in its best appearance of the year. It’s at opposition – it lines up opposite the Sun. It’s closest to Earth, so it shines brightest. And it’s in view all night. The giant planet looks like a bright golden star. It’s low in the east at nightfall, and climbs high across the south later on.

Script by Damond Benningfield