WEBVTT

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Howdy Star Gazers and welcome to this episode

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of Star Trails. My name is Drew, and I'll be

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your guide to the night sky for the week of March

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the 8th through the 14th. This week we continue

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our month -long exploration of our solar system.

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by leaving the warm terrarium of the inner planets

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for the deep freezer of the outer planets. In

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these far reaches, our sun is no longer a dominating

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presence, but a bright star among many, and the

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worlds we find here are as strange as they are

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lonely. Later in the show, I'll report on my

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efforts to observe a recent SpaceX rocket launch.

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We'll press forth into the next two chapters

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of Night Watch, And we'll look at what you can

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expect to see in the night sky this week. Whether

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you're tuning in from the backyard or the balcony,

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I'm glad you're here. So grab a comfortable spot

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under the night sky and let's get started. Tonight

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we pick up where we left off in the last episode.

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The rusty deserts of Mars are fading in the rear

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-view mirror of our spaceship, and the sun begins

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to shrink ever so slightly into something less

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oppressive and more distant. Ahead of us lies

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the asteroid belt, not the chaotic pinball machine

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of science fiction, but a wide, mostly empty

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region stretching between Mars and Jupiter. If

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you could stand on Ceres, the largest object

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there, and it's now classified as a dwarf planet,

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you'd see a lonely landscape of ice and rock

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under a dimmer sun. The belt contains millions

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of objects, yes, but they're separated by vast

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distances. Once we clear that frontier, the solar

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system changes character. The outer planets are

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not simply bigger versions of the inner ones.

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They're a different category of existence. Jupiter

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announces itself long before you arrive. It's

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more massive than all the other planets combined.

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A gravitational monarch presiding over the outer

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solar system. It resides around 5 AU from the

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sun, or about 465 million miles. Its diameter

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could fit more than 11 Earths across. Its volume

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could swallow more than 1 ,300 Earths whole.

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And yet it's made mostly of hydrogen and helium.

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The same stuff as our Sun. Just not quite massive

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enough to ignite nuclear fusion. Sometimes people

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call it a failed star, but that's poetic shorthand.

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In reality, it would need about 80 times more

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mass to shine. Jupiter's atmosphere is a masterpiece

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of fluid dynamics. Cream and cinnamon -hued bands

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wrap around the globe, driven by jet streams

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moving hundreds of miles per hour. The Great

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Red Spot, a storm larger than Earth, has been

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raging for at least 350 years. It seems to be

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shrinking, but it's still a planetary -scale

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hurricane that refuses to die. Jupiter also radiates

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more heat than it receives from the Sun. Deep

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inside, gravitational compression slowly releases

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energy, as if the planet is still settling into

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itself. And then there are the moons. Four of

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them were spotted in 1610 by Galileo Galilei,

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Io, Europa, Ganymede, and Callisto. Tiny moving

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points of light that quietly proved not everything

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orbits Earth. Not surprisingly, we refer to these

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as the Galilean moons, and even a small scope

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will reveal them here on Earth. Io is the most

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volcanically active world in the solar system.

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Europa likely hides a global ocean beneath its

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icy shell, twice as much water as all of Earth's

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oceans combined. Ganymede is the largest moon

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in the solar system and has its own magnetic

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field. We've explored Jupiter extensively. Pioneer

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10 and 11 first passed by in the 1970s. Voyager

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1 and Voyager 2 gave us the iconic images that

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have defined our view of Jupiter for four decades.

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Galileo orbited the planet for eight years in

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the 1990s and early 2000s, and today Juno continues

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to dive over the poles, mapping gravity, magnetic

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fields, and peering deep beneath the clouds.

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Now let's drift outward another 400 million miles

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to the ringed planet. Saturn feels like Jupiter's

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more refined sibling. It's less massive, but

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visually unforgettable. Its rings stretch hundreds

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of thousands of miles wide, yet in places they're

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only tens of meters thick. Thinner than a football

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field is long. They're made of countless particles

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of ice and rock, each one following Kepler's

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laws with quiet obedience. Saturn's density is

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so low that, in theory, it would float in water,

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if you had an ocean large enough to hold a planet.

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Saturn deserves more than it has rings. That's

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like introducing Jimi Hendrix by saying he dabbled

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in guitar. So let's widen the lens. First, Saturn

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is not just a smaller Jupiter. It's structurally

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different in subtle but important ways. While

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both are gas giants, comprised mostly of hydrogen

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and helium, Saturn's core is proportionally larger

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relative to its total mass. That may tell us

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something about how and where it formed in the

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early solar system. Planet formation models suggest

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Saturn may have grown more slowly than Jupiter,

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accreting gas after Jupiter had already become

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the dominant gravitational bully. Now let's talk

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about those rings in more depth because they're

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not permanent. The rings are likely young on

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cosmic timescales. Current models suggest they

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may be only a hundred to four hundred million

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years old, possibly the remains of a shattered

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moon torn apart by tidal forces after wandering

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too close. When dinosaurs walked Earth, Saturn

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may have looked different in the sky. The rings

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are organized into major divisions, A, B, and

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C rings, with the prominent Cassini division

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separating A and B. That gap isn't empty. It's

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sculpted by gravitational resonances with Saturn's

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moons. In other words, the moons are choreographing

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the rings. Tiny shepherd moons like Prometheus

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and Pandora actively confine ring material, preventing

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it from dispersing. Even so, the rings are slowly

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dissolving. At current rates, they may vanish

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in a hundred million years or so. Saturn's North

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Pole hosts a bizarre persistent hexagonal storm

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system. It's not a trick of the eye, it's a stable

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wave pattern in the atmosphere, larger than Earth.

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Saturn currently holds the record for the most

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known moons, well over a hundred confirmed objects,

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though many are tiny captured rocks. Titan and

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Enceladus get the spotlight, but Iapetus is a

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wonder too. One hemisphere bright as snow, the

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other dark as coal. The yin -yang moon. The real

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golden age of Saturn exploration came with Cassini

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-Huygens. For 13 years, Cassini orbited Saturn,

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transforming it from a distant ringed icon into

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a richly detailed world. It watched seasons change.

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It flew through the rings. It revealed Enceladus

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spraying plumes of water vapor from its south

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pole. evidence of a subsurface ocean. It delivered

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the Huygens probe to Titan, where it parachuted

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down through a thick orange atmosphere and landed

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on a surface shaped by methane rain. Titan has

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lakes and rivers, weather, dunes, a hydrological

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cycle built not on water but on hydrocarbons.

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When Cassini ended its mission in 2017, it deliberately

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plunged into Saturn's atmosphere to avoid contaminating

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potentially habitable moons. A spacecraft choosing

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its own fiery end to protect alien oceans is

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poetic engineering. And now we reach the ice

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giants, Uranus and Neptune. It's wild to think

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that through most of my childhood, we didn't

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have any detailed images of either of these worlds.

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All the books I grew up reading just featured

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artist's renditions, and both planets today still

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remain some of the least imaged. Of the two,

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Uranus is the real oddball. It rotates on its

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side, tilted 98 degrees. It essentially rolls

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around the sun. Its seasons last about 20 years

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apiece. For decades at a time, one pole faces

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the sun in continuous daylight, while the other

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endures unbroken darkness. Its pale blue color

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comes from methane in its atmosphere, which absorbs

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red light and reflects blue. Beneath the atmosphere

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lies a mantle of super pressurized water, ammonia,

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and methane ice. Some models suggest that under

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those immense pressures, carbon could crystallize

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into diamonds that rain downward through the

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interior. That remains a working hypothesis,

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but it's consistent with high pressure physics

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experiments. Like Saturn, Uranus has a ring system,

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although they are very different in almost every

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way. They were discovered in 1977 during a stellar

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occultation experiment. Astronomers were watching

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Uranus pass in front of a distant star. Instead

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of the star dimming once as the planet moved

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across it, it flickered multiple times before

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and after the main event. That meant something

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thin and structured was blocking the starlight.

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That something turned out to be rings. Uranus'

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rings are narrow, dark, and composed mostly of

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relatively large particles mixed with radiation

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-processed material that makes them charcoal

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-colored. They don't shine so much as they lurk.

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There are currently 13 known rings, named mostly

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with Greek letters, alpha, beta, gamma, and so

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on, along with a few more recently discovered

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faint outer rings. Like Saturn's, Uranus's rings

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are shaped and maintained by shepherd moons.

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Because the planet is tilted on its side, the

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rings are tilted with it. So from Earth, over

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decades we see the ring system dramatically change

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orientation. Sometimes they're wide open and

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visible, and other times we see them nearly edge

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on and they almost disappear. During Uranus's

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equinox, which happens only twice every 84 Earth

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years, the sun shines directly on the ring plane.

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producing unusual lighting effects and stirring

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up dynamic changes in the system. Voyager 2 gave

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us our only close -up look in 1986, and at the

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time the rings looked simple and sparse. But

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modern observations from the Hubble Space Telescope

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and large ground -based telescopes have revealed

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faint dusty components and more complex structure

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than Voyager initially detected. There's never

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been a return mission to Uranus. We know considerably

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more about it than we did before the Voyager

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flyby, but much of it has remained a pale turquoise

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mystery. At nearly 2 billion miles away, the

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sun is just a bright point of light at Uranus.

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And Uranus moves slowly. It takes 84 Earth years

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to complete one orbit. That means since its discovery

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in 1781 by William Herschel, Uranus has only

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completed a little more than two full orbits

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around the sun. Neptune lies even farther out,

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nearly 3 billion miles from the sun. It was the

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first planet discovered by mathematics before

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observation. Astronomers noticed irregularities

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in Uranus's orbit and predicted another world

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must be tugging at it. They calculated where

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it should be. Then they looked, and in 1846 they

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found it. It takes Neptune 165 Earth years to

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complete one orbit. It completed its first full

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orbit since discovery in 2011. Neptune's beautiful

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blue color comes from methane in its atmosphere,

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but it's a deeper, more vivid blue than Uranus.

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That difference likely comes from subtle atmospheric

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chemistry and haze layers we still don't fully

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understand. Neptune is also wildly dynamic for

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such a distant cold world. Its winds are the

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fastest in the solar system, reaching more than

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1200 miles per hour. That's supersonic, in a

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place where temperatures hover around minus 350

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degrees Fahrenheit. Neptune radiates more heat

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than it receives from the Sun, much like Jupiter.

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Its interior is still warm from formation. Triton

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is Neptune's largest moon and likely a captured

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Kuiper belt object. It orbits backwards, which

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is a huge clue that it didn't form alongside

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Neptune. As for exploration, Neptune has been

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visited exactly once. Voyager 2 flew past in

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August 1989. It revealed the Great Dark Spot,

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a storm similar to Jupiter's Red Spot, along

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with a ring system. After that brief encounter,

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Voyager kept going. Since then, it's only been

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studied by Hubble and some ground -based observatories,

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leaving a lot of unanswered questions. The outer

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planets hold most of the mass and angular momentum

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of our solar system. They sculpt cometary paths.

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They influence the asteroid belt. They may have

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helped make Earth stable enough for life. And

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yet, in terms of direct exploration, only Jupiter

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and Saturn have received sustained attention.

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Uranus and Neptune remain frontier worlds. There

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are serious proposals right now for a dedicated

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Uranus orbiter, but nothing has been launched

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yet. In some ways, the outer solar system still

00:15:45.899 --> 00:15:49.460
feels like it's stuck in the 1970s. And that's

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astonishing. When you step outside this evening

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and see Jupiter and Saturn blazing in the twilight,

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you're looking at a system of worlds we've actually

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visited. And beyond it lie two giants we've barely

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touched. We've mapped Mars with rovers and drones.

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We've landed on comets, but the ice giants remain

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largely unexplored. That should humble us a little,

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and maybe excite us. As we step back from this

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tour of the outer planets, it's natural to ask

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a bigger question. Why are the worlds closest

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to the sun small and rocky, while the outer planets

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are enormous spheres of gas and ice? The answer

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goes all the way back to the birth of the solar

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system, about 4 .6 billion years ago. At that

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time, the young sun was surrounded by a vast

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rotating disk of gas and dust. Close to the sun,

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temperatures were extremely high. In that hot

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inner region, only heavy materials like iron,

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nickel, and rocky minerals could condense into

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solid grains. Lighter substances, things like

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water, methane, and ammonia, remained vaporized.

00:17:05.509 --> 00:17:08.430
That meant the inner planets formed from relatively

00:17:08.430 --> 00:17:11.890
limited ingredients, building small, dense, rocky

00:17:11.890 --> 00:17:15.430
worlds like Mercury, Venus, Earth, and Mars.

00:17:16.170 --> 00:17:19.250
Farther from the sun, however, temperatures dropped

00:17:19.250 --> 00:17:22.670
dramatically. Beyond a certain distance, what

00:17:22.670 --> 00:17:26.190
astronomers call the frost line, water and other

00:17:26.190 --> 00:17:30.069
compounds could freeze into solid ice. Suddenly,

00:17:30.170 --> 00:17:33.009
there was far more material available to build

00:17:33.009 --> 00:17:37.710
planets. With ice joining rock and metal, planetary

00:17:37.710 --> 00:17:40.369
embryos in the outer solar system could grow

00:17:40.369 --> 00:17:43.769
much larger. Once these growing worlds became

00:17:43.769 --> 00:17:46.890
massive enough, their gravity began pulling in

00:17:46.890 --> 00:17:49.549
the surrounding hydrogen and helium gas from

00:17:49.549 --> 00:17:52.769
the disk, ballooning into the giant planets we

00:17:52.769 --> 00:17:56.859
see today. So the solar system naturally divided

00:17:56.859 --> 00:17:59.519
itself into two very different neighborhoods

00:17:59.519 --> 00:18:03.140
The inner region gave rise to small terrestrial

00:18:03.140 --> 00:18:06.980
planets made mostly of rock and metal While the

00:18:06.980 --> 00:18:10.180
cooler outer region produced the giant planets

00:18:10.180 --> 00:18:13.460
Jupiter and Saturn with their vast envelopes

00:18:13.460 --> 00:18:16.799
of hydrogen and helium and Uranus and Neptune

00:18:16.799 --> 00:18:20.000
with interiors rich and frozen compounds like

00:18:20.000 --> 00:18:24.539
water methane and ammonia All the planets, in

00:18:24.539 --> 00:18:27.460
a way, represent the structure of the original

00:18:27.460 --> 00:18:30.920
disk that formed our solar system. It's a fossil

00:18:30.920 --> 00:18:34.099
record of temperature, chemistry, and gravity

00:18:34.099 --> 00:18:57.259
written across billions of miles of space. After

00:18:57.259 --> 00:18:59.720
a quick break, we'll be back to discuss what

00:18:59.720 --> 00:19:02.579
you can actually see in this week's sky and how

00:19:02.579 --> 00:19:05.839
to spot these distant planets for yourself. Stay

00:19:05.839 --> 00:19:21.259
with us. Welcome back. Before we get into this

00:19:21.259 --> 00:19:24.380
week's sky, I have a quick observation report.

00:19:24.680 --> 00:19:28.359
Last week, a series of SpaceX launches were carried

00:19:28.359 --> 00:19:32.380
out from Cape Canaveral to deliver Starlink satellites

00:19:32.380 --> 00:19:35.500
into orbit. Some of these launches were in the

00:19:35.500 --> 00:19:38.700
evening or early morning, which means folks along

00:19:38.700 --> 00:19:42.279
the eastern seaboard hundreds of miles away can

00:19:42.279 --> 00:19:44.960
see them soaring into orbit if conditions are

00:19:44.960 --> 00:19:48.420
right. These launches weren't even on my radar

00:19:48.420 --> 00:19:51.400
until my brother -in -law, Chris, shared a post

00:19:51.400 --> 00:19:54.690
with me on Sunday afternoon. With nothing better

00:19:54.690 --> 00:19:57.869
to do, we decided to find a nice high elevation

00:19:57.869 --> 00:20:00.509
with an eastern view of the sky and see if we

00:20:00.509 --> 00:20:04.269
could spot a Falcon 9 rocket. We arrived at the

00:20:04.269 --> 00:20:08.630
site around 940 for the nearly 10pm launch. We

00:20:08.630 --> 00:20:12.089
both had the SpaceX live feed on our phones so

00:20:12.089 --> 00:20:15.230
we could hear the countdown and launch. About

00:20:15.230 --> 00:20:18.369
30 seconds after launch, looking south, Chris

00:20:18.369 --> 00:20:21.849
thought he spotted a red dot making its way upward

00:20:21.849 --> 00:20:25.869
into the east. then we didn't see anything. Some

00:20:25.869 --> 00:20:28.470
moments passed and then to the east and some

00:20:28.470 --> 00:20:31.750
30 degrees off the horizon, we spotted a bright

00:20:31.750 --> 00:20:35.450
reddish object, which morphed subtly for a few

00:20:35.450 --> 00:20:38.470
seconds, then winked out as fast as it appeared.

00:20:39.049 --> 00:20:42.269
It didn't look like the plumes we normally associate

00:20:42.269 --> 00:20:45.650
with SpaceX launches. We think the significant

00:20:45.650 --> 00:20:48.990
cloud cover may have affected our view, but based

00:20:48.990 --> 00:20:52.130
on Chris's initial observation and the direction

00:20:52.130 --> 00:20:54.640
it was heading, We're pretty certain we saw the

00:20:54.640 --> 00:20:58.500
rocket, 20 stories of fire and fury climbing

00:20:58.500 --> 00:21:02.859
into space at 17 ,000 miles per hour. Several

00:21:02.859 --> 00:21:05.720
days later, another Falcon took flight in the

00:21:05.720 --> 00:21:08.779
pre -dawn hours, and local observers captured

00:21:08.779 --> 00:21:11.859
some really stunning images of the rocket's plume

00:21:11.859 --> 00:21:15.759
as it blasted across the sky, backlit high in

00:21:15.759 --> 00:21:18.660
the atmosphere by the sun before it peeked over

00:21:18.660 --> 00:21:22.599
the horizon. Sadly, I wasn't awake for that launch.

00:21:23.000 --> 00:21:25.900
From now on, I'm going to make it a point to

00:21:25.900 --> 00:21:28.200
routinely check out what's launching from the

00:21:28.200 --> 00:21:32.119
Cape, using a website like Space Flight Now to

00:21:32.119 --> 00:21:35.119
see what's on deck. I'll include a link to that

00:21:35.119 --> 00:21:38.720
in the show notes. If there's an evening or nighttime

00:21:38.720 --> 00:21:41.319
launch window and you live in the viewable zone,

00:21:41.500 --> 00:21:44.240
it could make for a nice observation or even

00:21:44.240 --> 00:21:47.819
a photo op. Keep in mind the Kennedy Space Center

00:21:47.819 --> 00:21:51.690
isn't the only NASA launch pad. West coasters

00:21:51.690 --> 00:21:55.009
can try viewing rockets from Vandenberg Space

00:21:55.009 --> 00:21:58.829
Force Base in California. Farther up the East

00:21:58.829 --> 00:22:02.009
Coast, Wallops Flight Facility on the coast of

00:22:02.009 --> 00:22:05.730
Virginia is used for supply missions to the ISS.

00:22:06.569 --> 00:22:10.369
Alaska has a spaceport, and SpaceX's private

00:22:10.369 --> 00:22:14.440
launch site is in South Texas. There's surprisingly

00:22:14.440 --> 00:22:18.579
a lot of rocket action, so keep an eye on spaceflight

00:22:18.579 --> 00:22:21.319
now and maybe you can catch a launch from the

00:22:21.319 --> 00:22:24.440
Cape or from one of these alternate locations.

00:22:31.019 --> 00:22:33.900
Now, let's see what's in the sky above our own

00:22:33.900 --> 00:22:37.559
backyard this week. First, a quick note about

00:22:37.559 --> 00:22:41.319
daylight saving time. Clocks sprung forward one

00:22:41.319 --> 00:22:44.299
hour this morning. That pushes darkness later

00:22:44.299 --> 00:22:47.880
into the evening. Your best deep sky observing

00:22:47.880 --> 00:22:51.400
window will now start later after sunset, even

00:22:51.400 --> 00:22:54.759
as overall night length slowly increases toward

00:22:54.759 --> 00:22:58.980
the spring equinox on March 20. This week the

00:22:58.980 --> 00:23:02.099
moon is still in its waning gibbous to waning

00:23:02.099 --> 00:23:05.940
crescent phase. By March 14, it's a thin crescent

00:23:05.940 --> 00:23:09.400
with about 20 % illumination. Perfect for viewing

00:23:09.400 --> 00:23:12.500
surface detail near the terminator with binoculars

00:23:12.500 --> 00:23:16.519
or a telescope. After sunset in the western sky,

00:23:17.000 --> 00:23:20.059
brilliant Venus dominates low over the horizon.

00:23:20.640 --> 00:23:23.819
It's the brightest star you'll see after dusk.

00:23:24.059 --> 00:23:26.700
And early in the week you might spot Saturn just

00:23:26.700 --> 00:23:29.859
above or beside it. A visual pairing that will

00:23:29.859 --> 00:23:32.920
linger near the western horizon for several evenings

00:23:32.920 --> 00:23:37.359
as the planets slowly separate. A pair of binoculars

00:23:37.359 --> 00:23:40.599
will show them together easily, and around tonight

00:23:40.599 --> 00:23:44.559
or tomorrow that conjunction is tightest. In

00:23:44.559 --> 00:23:47.619
the southern evening sky, high above the horizon,

00:23:48.099 --> 00:23:51.359
Jupiter shines like a beacon. It's visible well

00:23:51.359 --> 00:23:54.200
after dark at this time of year and doesn't set

00:23:54.200 --> 00:23:57.559
until the late night hours. Its steady bright

00:23:57.559 --> 00:24:00.500
light makes it excellent for telescopic views.

00:24:00.900 --> 00:24:04.519
The Galilean moons and cloud belts are easy pickings.

00:24:04.839 --> 00:24:08.180
Mercury will be very low after sunset early in

00:24:08.180 --> 00:24:11.460
this window and quickly lost to twilight glow.

00:24:12.160 --> 00:24:15.039
It re -emerges in the morning sky later in March.

00:24:15.799 --> 00:24:18.839
Mars remains too close to the Sun for effective

00:24:18.839 --> 00:24:22.960
evening observing right now. Uranus is technically

00:24:22.960 --> 00:24:26.240
still placed in western Taurus and can be tracked

00:24:26.240 --> 00:24:29.700
down in binoculars or a small scope if the moon

00:24:29.700 --> 00:24:33.230
hasn't risen and your sky is dark. But Neptune

00:24:33.230 --> 00:24:35.789
is too close to conjunction with the Sun to be

00:24:35.789 --> 00:24:39.750
seen this week. Now let's talk deep sky objects.

00:24:40.470 --> 00:24:43.309
March evenings are rich with open star clusters

00:24:43.309 --> 00:24:46.670
and faint nebula that reward patients and optics,

00:24:47.029 --> 00:24:50.849
especially once the moon sets. The Hyades cluster

00:24:50.849 --> 00:24:54.650
near Aldebaran and Taurus is a sprawling binocular

00:24:54.650 --> 00:24:58.329
-friendly grouping. Look for the broad V of stars

00:24:58.329 --> 00:25:01.859
that makes up the head of the bull. The Rosette

00:25:01.859 --> 00:25:05.380
nebula and its embedded cluster in Monoceros

00:25:05.380 --> 00:25:09.000
is a favorite for long exposures and narrow band

00:25:09.000 --> 00:25:12.500
imaging. A pair of binoculars under dark skies

00:25:12.500 --> 00:25:15.359
will show the cluster and a camera will begin

00:25:15.359 --> 00:25:19.440
to tease out nebulosity. The Beehive cluster

00:25:19.440 --> 00:25:23.839
M44 in Cancer sits higher in the late evening

00:25:23.839 --> 00:25:27.579
once the moon dips below the horizon. This object

00:25:27.579 --> 00:25:30.640
is beautiful through small scopes and even in

00:25:30.640 --> 00:25:34.480
urban skies. While there's no major meteor shower

00:25:34.480 --> 00:25:37.619
peaking this week, a few minor streams may be

00:25:37.619 --> 00:25:41.059
detectable after midnight under truly dark skies.

00:25:41.859 --> 00:25:44.640
Finally, don't forget the spring constellations

00:25:44.640 --> 00:25:48.519
rising in the east late evening. Leo, with its

00:25:48.519 --> 00:25:52.259
graceful sickle, and regal regulus, and Cancer

00:25:52.259 --> 00:25:55.819
just above, are home to loose stellar groupings.

00:25:56.160 --> 00:25:58.940
These aren't the obvious constellations like

00:25:58.940 --> 00:26:02.559
Orion or Ursa Major, but they'll reward viewers

00:26:02.559 --> 00:26:10.599
who take time with their charts and optics. For

00:26:10.599 --> 00:26:12.980
this week's book club segment, we're looking

00:26:12.980 --> 00:26:17.099
at chapters 6 and 7 of Nightwatch, covering the

00:26:17.099 --> 00:26:20.809
deep sky and the planets. And what I appreciate

00:26:20.809 --> 00:26:23.849
most about these chapters is that Terrence Dickinson

00:26:23.849 --> 00:26:26.109
continues what he's done throughout the book.

00:26:26.529 --> 00:26:30.630
He manages expectations. In chapter 6, when he

00:26:30.630 --> 00:26:34.349
describes deep sky objects like galaxies, nebula,

00:26:34.630 --> 00:26:37.829
and globular clusters, he tells you plainly what

00:26:37.829 --> 00:26:40.970
they actually look like in the eyepiece. They're

00:26:40.970 --> 00:26:44.589
dim, subtle, often colorless, and that's just

00:26:44.589 --> 00:26:48.759
how our eyes work. Under low light, our eyes

00:26:48.759 --> 00:26:53.140
rely mostly on rod cells. Rods are incredibly

00:26:53.140 --> 00:26:55.920
sensitive to faint light, which is why they allow

00:26:55.920 --> 00:26:58.660
us to see these ghostly smudges in the first

00:26:58.660 --> 00:27:02.819
place. But rods don't detect color well. The

00:27:02.819 --> 00:27:06.420
cone cells that do perceive color require much

00:27:06.420 --> 00:27:09.390
brighter light to activate. So when you look

00:27:09.390 --> 00:27:12.769
at the Orion Nebula or the Andromeda Galaxy through

00:27:12.769 --> 00:27:15.210
a telescope, you're not seeing the saturated

00:27:15.210 --> 00:27:18.990
pinks and blues of astrophotography. You're seeing

00:27:18.990 --> 00:27:21.829
what the human visual system can gather in a

00:27:21.829 --> 00:27:25.549
fraction of a second. A camera can collect photons

00:27:25.549 --> 00:27:29.690
for minutes. It can stack exposures for hours.

00:27:30.170 --> 00:27:34.640
Your retina resets continuously. Dickinson explains

00:27:34.640 --> 00:27:37.579
this, and I think that's crucial. I think new

00:27:37.579 --> 00:27:40.500
astronomers expect the sky to look like processed

00:27:40.500 --> 00:27:44.839
long exposure images. But visual astronomy is

00:27:44.839 --> 00:27:48.259
quieter than that. It's about contrast, texture,

00:27:48.500 --> 00:27:51.700
and shape. It's about learning to recognize faint

00:27:51.700 --> 00:27:55.119
structure at the edge of perception. And then

00:27:55.119 --> 00:27:57.579
Dickinson gives us something very practical.

00:27:58.039 --> 00:28:02.460
Maps. The deep sky charts in chapter 6 are clean,

00:28:02.859 --> 00:28:05.960
readable, and focused. They highlight specific

00:28:05.960 --> 00:28:09.700
objects. They indicate magnitude. They note what

00:28:09.700 --> 00:28:12.900
size instrument might be needed. They help you

00:28:12.900 --> 00:28:15.720
plan a session instead of overwhelming you with

00:28:15.720 --> 00:28:19.440
thousands of targets. There's something philosophical

00:28:19.440 --> 00:28:22.380
there. He's not encouraging you to conquer the

00:28:22.380 --> 00:28:25.160
sky. He's encouraging you to spend time with

00:28:25.160 --> 00:28:28.980
it. Then in chapter 7, when he turns to the planets,

00:28:29.059 --> 00:28:32.500
he does something similar. Again, he calibrates

00:28:32.500 --> 00:28:36.720
expectations. Saturn will not look like a glossy

00:28:36.720 --> 00:28:40.819
NASA poster. Mars won't resemble a spacecraft

00:28:40.819 --> 00:28:45.099
mosaic. Jupiter's belts may be subtle. Features

00:28:45.099 --> 00:28:48.539
will shift from night to night. And that's the

00:28:48.539 --> 00:28:52.759
point. Planets reward repeated observation. You

00:28:52.759 --> 00:28:55.839
begin to notice the tilt of Saturn's rings changing

00:28:55.839 --> 00:29:00.460
over years, the shrinking and expanding of Mars's

00:29:00.460 --> 00:29:04.240
polar caps, the steady dance of Jupiter's moons.

00:29:04.819 --> 00:29:07.779
Patience is the key here. I think both of these

00:29:07.779 --> 00:29:11.339
chapters serve as nice companions to this podcast,

00:29:11.880 --> 00:29:14.140
especially the chapter on the planets, since

00:29:14.140 --> 00:29:17.539
we've been discussing them all month long. We

00:29:17.539 --> 00:29:20.779
mention Deep Sky objects on nearly every episode,

00:29:21.140 --> 00:29:23.980
and while smartphone apps and computer databases

00:29:23.980 --> 00:29:27.400
make it easy to locate and track these objects,

00:29:27.920 --> 00:29:31.180
those great maps included in Nightwatch are really

00:29:31.180 --> 00:29:34.059
helpful for planning and laying out what's what

00:29:34.059 --> 00:29:37.059
and where it's located in relation to common

00:29:37.059 --> 00:29:40.440
constellations. We'll be back in two weeks with

00:29:40.440 --> 00:29:48.700
a discussion on the next two chapters. That's

00:29:48.700 --> 00:29:50.920
going to do it for this week. If you found this

00:29:50.920 --> 00:29:53.339
episode interesting, please share it with a friend

00:29:53.339 --> 00:29:56.019
who might enjoy it. The easiest way to do that

00:29:56.019 --> 00:29:59.480
is by sending folks to our website, StarTrails

00:29:59.480 --> 00:30:02.839
.show. And if you'd like to support the show,

00:30:03.079 --> 00:30:05.400
use the link on the site to buy me a coffee.

00:30:05.759 --> 00:30:09.460
That really helps. Be sure to follow Star Trails

00:30:09.460 --> 00:30:12.740
on Blue Sky and YouTube. Links are in the show

00:30:12.740 --> 00:30:15.799
notes. Until we meet again beneath the stars.

00:30:16.079 --> 00:30:17.440
Clear skies everyone!
