WEBVTT

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Howdy Star Gazers, and welcome to this episode

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of Star Trails. I'm Drew, and I'll be your guide

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to the night sky for the week starting March

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the 16th through the 22nd. This week we say goodbye

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to some visible planets, at least for a little

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while. Leo roars into the night sky, resplendent

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with its fascinating triplet of galaxies. And

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this week's equinox means that spring has officially

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arrived. So grab a comfortable spot under the

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night sky and let's get started. Before we get

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into the main program, I'd like to take a moment

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to answer a listener's request. A few days ago,

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a very generous anonymous listener sent the podcast

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a donation and wrote in with an intriguing question.

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Here's what they asked. Why do you choose to

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call frozen water water ice and not just ice?

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I grew up in greater Philadelphia and every time

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you say water ice I wonder lemon or cherry Okay,

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so I love this question because I was just in

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Philadelphia last week and sadly I didn't get

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any water ice Although I did enjoy maybe the

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best cheese steak I've ever had in a dive bar

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near Fairmount But seriously, you've picked up

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on an important distinction that astronomers

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make when talking about ice in space. Here on

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Earth when we say ice, we almost always mean

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frozen water, H2O. But out in the cosmos, ice

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isn't just limited to water. In space, temperatures

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can be incredibly low, allowing many different

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substances to freeze into solid form. Some of

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the most common space ices include frozen methane,

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ammonia, carbon dioxide, often called dry ice

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on Earth, and even nitrogen. It's safe to say

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you probably wouldn't want to eat any of these

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ices. Since all of these materials can exist

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in a frozen state, astronomers use the term water

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ice specifically to refer to frozen H2O. A great

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example of why this distinction matters are the

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polar ice caps on Mars. Both of Mars' poles have

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layered ice caps, but they aren't made of just

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one type of ice. The main component is water

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ice, similar to Earth's polar ice caps. However,

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during the Martian winter, the caps are also

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coated with a seasonal layer of frozen carbon

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dioxide, which sublimates into gas in the warmer

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seasons. This seasonal cycle is a key part of

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Martian weather patterns. The same kind of distinction

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applies when we study icy moons, comets, and

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distant planets. Saturn's moon, Titan, for instance,

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has surface ice, but much of it is actually frozen

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hydrocarbons like methane. Meanwhile, Europa

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and Enceladus are known for their subsurface

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oceans of liquid water beneath a thick crust

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of water ice, which is why they're such exciting

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places to study for potential extraterrestrial

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life. So, in astronomy, we clarify by saying

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water ice to be precise about what kind of ice

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we're talking about. It's just one of the many

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frozen substances out there in the cold reaches

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of space. And if we ever find blue raspberry

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water ice on another planet, it'll certainly

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be the discovery of a century. Thanks again for

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that question and especially for the thoughtful

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donation. I welcome anyone to write in or just

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let me know what you've been enjoying in the

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night sky. If you feel inclined to donate, check

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the link in the show notes or on the show website.

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Scroll down on the homepage until you see the

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donate button. I hope everyone had the opportunity

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to see the stunning full lunar eclipse early

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Friday morning. At my location, we'd had clouds

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all day, but the sky cleared around 9 p .m. and

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the full moon was extremely bright. Some hours

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later, I went outside around 2 .30 a .m. to check

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out the eclipse, which was nearing totality.

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The moon was almost right overhead and all the

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bright moonlight from earlier was gone. The moon

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was a subtle red color with a slightly brighter

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coloring along the northern limb. Through binoculars,

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it almost reminded me of Mars with its red shading

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and ice caps. Every time I've watched the total

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lunar eclipse, at least one side of the moon

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seems brighter than the rest. Apparently, this

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is owing to the Earth's uneven shadow density.

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The Earth's umbra is not an evenly distributed,

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perfectly dark shadow. The outer edges of the

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umbra allow more sunlight to refract through

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the Earth's atmosphere, meaning parts of the

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moon near the umbral edge receive more scattered

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light than the deeper central regions. Also,

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the way our atmosphere filters the sunlight could

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cause some shadow variations. The red color of

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the moon during totality comes from Rayleigh

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scattering, the same effect that makes sunrises

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and sunsets red. Earth's atmosphere bends sunlight

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around the planet, filtering out shorter blue

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and green wavelengths and casting a reddish hue

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onto the moon. However, the amount of dust, pollution,

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or clouds in Earth's atmosphere at the time of

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the eclipse can vary, causing uneven filtering.

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Some areas of the moon might receive slightly

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more light than others, leading to patches of

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dim orange or yellow instead of deep red. I was

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also struck by how small the moon looks right

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now. Back around the end of last year, when we

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had several consecutive super moons, the moon

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was noticeably larger and more dominant in the

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sky. Of course, the moon's distance to Earth

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changes throughout the year, owing to its elliptical

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orbit. The moon will reach Apogee, its point

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farthest from Earth, on March 17th. So it's much

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smaller in the sky right now. The difference

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between Apogee and Perigee, the closest point

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to Earth, can be more than 30 ,000 miles, so

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the difference is significant. Also, its high

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point in the sky during the eclipse means that

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we didn't experience the so -called moon illusion,

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where it seems larger in the sky as it gets closer

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to the horizon. If you saw the eclipse, I'd love

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to hear your observations, so visit StarTrails

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.Show and send me a report. With the eclipse

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behind us, we begin the week with the moon in

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a waning gibbous phase, just following last week's

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full moon. It's still nearly full early in the

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week with nearly 90 % illumination. But by Saturday,

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we'll reach the last quarter moon. At this phase,

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half of the moon appears illuminated, but only

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in the morning sky. That means deep sky observers

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still enjoy darker skies to work with at least

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until 3 a .m. or so. If you're into astrophotography,

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the last quarter is a great time to capture the

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moon's rugged terrain. With the light coming

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in from the side, you'll get great contrast on

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lunar mountains and craters along the terminator.

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That's the line between night and day on the

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moon's surface. Now onto the planets. After the

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recent spectacular parade of planets that gave

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some observers the chance to see all the visible

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planets lined up across the sky, we've basically

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lost three of them. Mercury is once again too

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close to the Sun, and it's joined by Venus and

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Saturn. All three bodies are bunched up with

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the Sun this week. You may still be able to catch

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a glimpse of Mercury and Venus tonight, just

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after sunset, and very low on the western horizon.

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But as the week progresses, our two interplanetary

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companions will dip closer to the horizon each

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night at sunset, until we can't see them anymore.

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By the week's end, Venus will be ahead of the

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Sun, and by next week will transition to a morning

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star, rising in the east just before the Sun.

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This transformation happens roughly every 19

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months as Venus moves between Earth and the Sun

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in its orbit. We've been enjoying the presence

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of Venus in the evening sky since last fall,

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the third brightest object in the sky after the

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Sun and Moon. By the month's end, you'll need

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to be an early riser to catch its brilliance

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in the pre -dawn sky. Jupiter, the king of planets,

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is still high and bright in the early evening.

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Located in the constellation Taurus, and with

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Venus gone, it claims its place as the brightest

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object after the moon. Look for it near Aldebaran,

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the orange giant star that marks the eye of the

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bull. If you have a telescope, this is a great

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time to check out Jupiter's four largest moons,

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Io, Europa, Ganymede, and Callisto, easily visible

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as tiny points of light near the gas giant. Mars

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is nearby, sitting in Gemini, close to the twin

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stars Castor and Pollux. Unlike the flickering

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glow of those stars, Mars has a distinct and

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constant reddish hue. Now, let's turn our attention

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to some of the constellations that dominate the

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night sky in March. Taurus is a powerhouse this

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season, home to some of the best known deep -sky

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objects. Along with Aldebaran, look for Messier

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45, the Pleiades. That's the little cluster of

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stars that looks like a tiny dipper. In mythology,

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the Pleiades were seven sisters pursued by Orion.

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And in modern astronomy, this cluster is one

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of the closest and brightest open star clusters

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to Earth. Even without any equipment, the Pleiades

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appears as a small hazy patch in the constellation

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Taurus. Most people can see six or seven stars

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under dark skies. Interestingly, one of the best

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views of the Pleiades comes with binoculars.

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The cluster is larger than the full moon, so

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it's actually too spread out to fit entirely

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in most telescopic views. With binoculars, the

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brightest stars become distinct, each glowing

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in shades of blue -white. You'll also start to

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notice that the cluster contains dozens of fainter

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stars that blend into the glow when seen with

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the naked eye. A small telescope will show even

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more stars, possibly up to 100 members of the

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cluster scattered across the field of view. It's

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best to use a low -power, wide -field eyepiece.

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If you're in an extremely dark location, you

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might catch a glimpse of a faint bluish reflection

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nebula. This is leftover dust that the cluster

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is currently passing through, reflecting the

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light of its young, hot stars. It's faint, so

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long exposure astrophotography does a much better

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job of bringing it out in visual observation.

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Fun fact, while the Pleiades is generally called

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the Seven Sisters, in Japanese it's known as

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Subaru. And if you look closely at the Subaru

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car logo, you'll see a stylized version of the

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cluster. Leo the lion is another March favorite.

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This constellation rises in the east in the evening

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and is easy to spot thanks to its backward question

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mark shape. That's called the sickle. In ancient

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cultures, Leo was often associated with royalty,

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strength, and the sun, which is fitting since

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it's a sign that warmer days are ahead. The brightest

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star in Leo is Regulus, a bluish -white star

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that's about 79 light years away. And here's

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another fun fact. It actually spins so fast that

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it's not quite a sphere, but slightly flattened.

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One of the highlights of LEO is the LEO Triplet,

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a stunning group of three spiral galaxies, Messier

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65, Messier 66, and NGC 3628, all located about

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35 million light years away. M65 is slightly

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tilted toward us, giving it a classic spiral

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shape. It has a yellowish core, meaning it has

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older stars, but also some dust lanes where new

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stars are forming. M66 is more distorted, likely

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due to gravitational interactions with its neighboring

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galaxies. It has strong spiral arms and huge

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dust clouds. NGC 3628, also called the Hamburger

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Galaxy, is the third member of the triplet. This

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galaxy has a thick dust lane cutting across it,

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making it look like a cosmic sandwich. It's a

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little fainter than M65 and M66, but if you're

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in a dark location with a telescope, you might

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catch it. The Leo triplet is an active, dynamic

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group, meaning these galaxies are pulling and

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warping each other, due to their gravitational

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interactions. They may eventually merge millions

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of years from now, but for now they make a spectacular

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sight for sky watchers. To find them, look just

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below the lion's belly near the star Cherton.

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If you have a telescope with a wide field of

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view, you can see all three galaxies together

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in a single frame. A notable astronomical event

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this week is the Spring Equinox, happening on

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March 20. Twice a year, Earth's tilt lines up

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perfectly perpendicular to the Sun. That means

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for a brief moment, day and night are nearly

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equal all over the world. The word equinox comes

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from the Latin for equal night. This is the official

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start of spring in the Northern Hemisphere, and

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cultures around the world have celebrated it

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for millennia. Ancient civilizations like the

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Mayans built entire structures, like the temple

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of Kukulkan at Chichen Itza, that align with

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the Sun on the equinox, creating a serpent -like

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shadow on the pyramid's steps. Astronomically,

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the equinox is a halfway point. It's when the

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Sun crosses the celestial equator moving from

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the southern half of the sky into the northern

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half. From now on, our days will keep getting

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longer until we reach the summer solstice in

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June, when the sun is at its highest point. If

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you found this episode helpful, let me know and

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feel free to send in your questions and observations.

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The easiest way to do that is by visiting our

00:16:01.029 --> 00:16:05.529
website StarTrails .Show. This is also a great

00:16:05.529 --> 00:16:08.529
way to share the show with friends. Until next

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time, keep looking up and exploring the night

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sky. Clear skies everyone!
