Latest / Star Trails: From Backyard Astronomy to Cosmic Wonder / Urban Alignments and Cosmic Parking Spots
Transcript
- 0:07Howdy stargazers, and welcome to this episode
- 0:10of Star Trails. Drew here, and I'll be your guide
- 0:14to the night sky for the week starting June 1st
- 0:17through the 7th. This week, the rising summer
- 0:21triangle lets us know that warmer nights are
- 0:24ahead. We take a moment to explore a peculiar
- 0:27solar alignment in New York City known as Manhattan
- 0:32Hinge, and later we explore the parking lots
- 0:35of space known as the Lagrange Points. Whether
- 0:39you're tuning in from the backyard, the balcony,
- 0:42or just your imagination, I'm glad you're here.
- 0:45So find a cozy spot, let your eyes adjust, and
- 0:49let's see what the sky holds for us this week.
- 0:53The moon is currently waxing. Tonight it's in
- 0:57a crescent phase with about 6 % illumination.
- 1:01It will reach first quarter on June 3rd with
- 1:04the full moon arriving around the middle of next
- 1:07week. Venus is shining brilliantly at magnitude
- 1:11negative 4 and it's just reached its greatest
- 1:14western elongation, making it a prominent morning
- 1:18star in the eastern sky before sunrise. Saturn
- 1:22is still visible in the early morning sky, rising
- 1:26in the east during the predawn hours. While not
- 1:29as bright as Venus, it's distinguishable by its
- 1:32steady yellowish glow. Look westward after sunset
- 1:37tonight to spot a conjunction of the moon and
- 1:40Mars. The waxing crescent moon will appear close
- 1:44to Mars, offering a picturesque pairing for evening
- 1:47observers. Mercury is currently too close to
- 1:50the Sun to be easily observed, but it will become
- 1:53more visible in the evening sky later this month.
- 1:57As summer creeps closer, the night sky starts
- 2:00to show off its southern stars, and this week
- 2:03you'll have some real stunners to track down.
- 2:07Low in the southeast after dark, you'll spot
- 2:09the curve of Scorpius, one of the few constellations
- 2:13that actually looks like what it's named after.
- 2:16Its brightest star, Antares, whose name actually
- 2:20means rival of Mars, is a massive red supergiant
- 2:25nearing the end of its life, and like Mars, it
- 2:28glows with a deep, rusty hue. Just to the west
- 2:32of Antares is M4, a dense globular cluster that
- 2:37looks like a fuzzy star in binoculars. Right
- 2:40next door to Scorpius is Sagittarius, home to
- 2:44the famous teapot asterism. If you can trace
- 2:48the teapot shape, imagine steam rising from its
- 2:52spout. That glowing steam is actually the densest
- 2:56part of the Milky Way, and it's pointing straight
- 2:59toward the galactic core. Now, you can't see
- 3:02the center of the galaxy directly. It's hidden
- 3:05behind gas and dust. But you can look in the
- 3:08exact direction of it, which is kind of amazing.
- 3:12And right there, about 26 ,000 light years away,
- 3:16lies Sagittarius A, a supermassive black hole
- 3:21anchoring the Milky Way's spiral arms. The area
- 3:25around it is absolutely loaded with deep sky
- 3:29gems. There's M8, the Lagoon Nebula, a bright
- 3:34stellar nursery. M20, the Trifid Nebula, is a
- 3:38beautiful mix of newly born stars and dark dust.
- 3:43Also check out M22, one of the best globular
- 3:47clusters in the sky, and also easy to spot with
- 3:51binoculars. Even to the naked eye under dark
- 3:54skies, this part of the Milky Way looks puffier,
- 3:57brighter, and deeper. It's like the galaxy is
- 4:00exhaling. And of course, the summer triangle
- 4:04is rising. High in the east, later in the evening,
- 4:08you'll see three bright stars forming a giant
- 4:11triangle. Vega, Altair, and Deneb. The Triangle
- 4:16is up for most of the night and offers a gateway
- 4:19to other fun targets like the Ring Nebula M57
- 4:23in Lyra and the North America Nebula near Deneb.
- 4:35Have you ever seen the sun set perfectly between
- 4:39city buildings like it was aiming right down
- 4:42the street? If you were in New York City last
- 4:45week, you might have caught Manhattan Hinge.
- 4:49That's when the sun lines up just right with
- 4:51Manhattan's grid, beaming down the east -west
- 4:55streets like a spotlight. But if you missed it,
- 4:59and if you happen to be in New York City in a
- 5:01few weeks, you'll get another shot to see it.
- 5:05The next Manhattan Hinge is happening around
- 5:07July the 12th and 13th. And if you're nowhere
- 5:11near Manhattan, stick around because your city
- 5:14might have its own version of this urban sky
- 5:17alignment. So what exactly is Manhattan Hinge?
- 5:22It's a twice -a -year event when the setting
- 5:25sun aligns with Manhattan's slightly tilted street
- 5:29grid. The result is, for a few minutes, the sun
- 5:33drops directly between the buildings, lighting
- 5:35up the avenues in a perfect glowing frame. New
- 5:39York's street grid is rotated about 29 degrees
- 5:43off True East and West, so this solar alignment
- 5:47happens only when the Sun's path intersects that
- 5:50angle, once in late May and again in mid -July.
- 5:55Some top spots to view it include 42nd Street,
- 5:5934th Street, and 14th Street. The phenomenon
- 6:04was dubbed Manhattan Hinge by science educator
- 6:07Neil deGrasse Tyson, and that of course is a
- 6:10reference to Stonehenge, the prehistoric stone
- 6:14circle in England that forms a cosmic calendar,
- 6:18and it aligns with the summer solstice sunrise
- 6:21and winter solstice sunset. Stonehenge has modern
- 6:26pagans who gather to experience the solar phenomenon,
- 6:30while New York City has, well, taxis. New York
- 6:34isn't the only place that gets this light show.
- 6:37Cities like Chicago, Toronto, Montreal, Philadelphia,
- 6:42and Salt Lake City all experience similar events,
- 6:46sometimes at sunset, sometimes at sunrise, depending
- 6:49on their grid orientation. For example, Chicago
- 6:53has Chicago Hinge near the spring and fall equinoxes
- 6:57because its street grid runs true east to west.
- 7:02So, how can you tell if your city has a hinge
- 7:05of its own? This is where a little digital astronomy
- 7:08comes in handy. There's a great tool called the
- 7:11photographer's ephemeris, and it lets you map
- 7:15the sun's path for any date and place on Earth.
- 7:19You can overlay that info onto your city's street
- 7:22grid and figure out when the sun will align with
- 7:26your favorite thoroughfare. It's super useful
- 7:29if you're chasing that perfect golden hour photo
- 7:32or just want to know when your city might surprise
- 7:35you with a solar corridor. So maybe there's a
- 7:38hinge waiting just a few blocks from you. Let's
- 7:48shift gears a little from stargazing with your
- 7:51eyes to something that's mostly invisible but
- 7:55still incredibly important. Tonight, I want to
- 7:59take you behind the scenes of the solar system
- 8:01into the hidden architecture that holds things
- 8:04steady in space. We're talking about the Lagrange
- 8:08points, those weird gravitational sweet spots
- 8:12that make spaceflight smarter, smoother, and
- 8:16in some cases, just a little bit spooky. If you've
- 8:19never heard of them before, Lagrange points,
- 8:23sometimes just called L points, are specific
- 8:26spots in space where the gravity of two large
- 8:29objects, like the Earth and the Sun, balances
- 8:32out just right. So right, in fact, that a third,
- 8:36much smaller object, like a satellite, can just
- 8:40sort of hang out there, using no thrusters or
- 8:44any fuel. It just drifts along in harmony with
- 8:47the big cosmic players. So picture this, you've
- 8:51got the Earth orbiting the Sun, and both of them
- 8:54are tugging on a satellite with their combined
- 8:57gravity. Normally, that would yank the satellite
- 9:00around unpredictably, but at a Lagrange point,
- 9:04the gravitational pulls and the orbital motion
- 9:07all sync up perfectly, like a cosmic dance step
- 9:11where the satellite always lands right on the
- 9:14beat. There are five of these Lagrange points
- 9:17in any two -body system. Let's stick with the
- 9:20big show for now, the Earth -Sun system. L1 is
- 9:25for sun watchers. The first Lagrange point, L1,
- 9:29sits directly between Earth and the Sun. It's
- 9:33about a million miles from Earth, closer to the
- 9:36Sun than we are, but locked in Earth's orbital
- 9:39path. This is where we park solar observatories
- 9:42like SOHO and the Discover spacecraft because
- 9:46L1 gives them an uninterrupted view of the Sun,
- 9:50which is perfect for studying solar flares, sunspots,
- 9:53and space weather that can affect satellites
- 9:56and even power grids down here on Earth. It's
- 9:59the front row seat for solar drama, and it's
- 10:02always in the light. Now L2 is a nice place for
- 10:08deep space stargazers. L2 is located about a
- 10:12million miles away from Earth, but on the far
- 10:15side away from the Sun. This spot is special
- 10:18because it allows telescopes to stay in Earth's
- 10:21shadow, with the Sun, Earth, and Moon all behind
- 10:24them. That makes it incredibly cold and dark,
- 10:28just what you want for observing faint galaxies
- 10:31and distant stars. This is where the James Webb
- 10:35Space Telescope lives. Its mirrors and instruments
- 10:39are designed to pick up the faintest heat signatures
- 10:41in the universe, so it needs that cold, quiet
- 10:45neighborhood. Think of L2 as the astronomer's
- 10:48porch, but with the light turned off. L3 is sometimes
- 10:54called the phantom point. L3 sits on the far
- 10:58side of the Sun, directly opposite Earth. It's
- 11:01always hidden from our view. You can't see it
- 11:04from here, and that's what's given rise to all
- 11:07kinds of fun science fiction ideas like secret
- 11:10planets, alien outposts, or even doppelganger
- 11:14Earths hiding in the blind spot. But in real
- 11:18life, L3 isn't all that stable. If you tried
- 11:22to park a satellite there, it would eventually
- 11:24drift away. Think of L4 and L5 as the cosmic
- 11:29rest stops. These points form the tips of an
- 11:33equilateral triangle with the Earth and the Sun.
- 11:37That means they lead and trail Earth in its orbit
- 11:40about 60 degrees ahead of and behind. L4 and
- 11:45L5 are really stable. Objects placed there tend
- 11:49to stay put even if they get nudged a little.
- 11:52They often collect space debris, dust clouds,
- 11:56and even asteroids. Jupiter, for example, has
- 11:59thousands of asteroids camped out at its L4 and
- 12:03L5 points. Earth has a few too, though they're
- 12:07much smaller and harder to spot. Some scientists
- 12:10even speculate that alien probes, if they existed,
- 12:15would choose L4 or L5 as a parking spot. They're
- 12:19hidden, stable, and offer a great long -term
- 12:23view of Earth. So what makes these places so
- 12:26valuable? For one, they reduce the energy needed
- 12:30to keep spacecraft in a fixed position. That
- 12:34means less fuel, longer missions, and more stable
- 12:37instruments. And for future space infrastructure,
- 12:41things like observatories, solar power stations,
- 12:44or even planetary defense systems, Lagrange points
- 12:48offer premium real estate. They also give us
- 12:52strategic vantage points, whether we're monitoring
- 12:54solar storms, peering into deep space, or preparing
- 12:58for interplanetary travel. These points let us
- 13:01place our tools exactly where they'll be most
- 13:04effective. So the next time you hear about a
- 13:07new space telescope or satellite mission, listen
- 13:10closely and there's a good chance it's heading
- 13:13for one of these gravitational sweet spots. For
- 13:16the math of motion and the poetry of space come
- 13:19together just right. If the stars spoke to you
- 13:28this week or if a question's been on your mind,
- 13:30I'd love to hear it. Visit our website, StarTrails
- 13:34.Show, where you can contact me and explore past
- 13:38episodes. Be sure to follow us on Mastodon, Blue
- 13:42Sky, and YouTube. Links are in the show notes.
- 13:46Until we meet again beneath the stars, clear
- 13:48skies everyone.