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00:00:00 --> 00:00:02 Anna: G' day and welcome to Astronomy
00:00:02 --> 00:00:03 AstroDailyPod. I'm Anna.
00:00:03 --> 00:00:06 Avery: And I'm Avery. It's the weekend wrap for
00:00:06 --> 00:00:08 Saturday 8th August, and this is one of those
00:00:08 --> 00:00:11 rare weekends where the sky itself is the
00:00:11 --> 00:00:13 headline. We are four days out from a total
00:00:13 --> 00:00:16 solar eclipse and the peak of the Perseids
00:00:16 --> 00:00:17 landing on the very same night.
00:00:17 --> 00:00:20 Anna: We'll get you set for all of that in the sky
00:00:20 --> 00:00:22 watch at the end. Both hemispheres, proper
00:00:22 --> 00:00:25 local times and one eye safety rule.
00:00:25 --> 00:00:27 None of us are allowed to skip.
00:00:27 --> 00:00:30 But we start where the whole week has quietly
00:00:30 --> 00:00:31 been pointing at the sun.
00:00:32 --> 00:00:34 Avery: Then, um, three storeys at the find the week.
00:00:34 --> 00:00:37 A rocket stage that finally hit The Moon, a
00:00:37 --> 00:00:39 48 year old spacecraft that just bought
00:00:39 --> 00:00:41 itself another year of life, and the rescue
00:00:41 --> 00:00:43 mission that spent, uh, the week rescuing
00:00:43 --> 00:00:45 itself. Let's go.
00:00:45 --> 00:00:47 Anna: Here's the question that sounds simple and
00:00:47 --> 00:00:50 isn't. What does the surface of the sun
00:00:50 --> 00:00:53 actually look like up close? Not the
00:00:53 --> 00:00:56 postcard, the fine detail right down at
00:00:56 --> 00:00:58 the scale where the physics happens. This
00:00:58 --> 00:01:01 week for the first time, we got to see it.
00:01:01 --> 00:01:04 And the answer is it's covered in whirlpools.
00:01:04 --> 00:01:06 Avery: Whirlpools on the sun.
00:01:07 --> 00:01:09 Anna: Tiny ones, some only about 20
00:01:09 --> 00:01:12 kilometres across, which on the sun is almost
00:01:12 --> 00:01:15 microscopic. In a paper published Wednesday
00:01:15 --> 00:01:18 in Nature, a team led by David
00:01:18 --> 00:01:20 Kureads at the U.S. national Solar
00:01:20 --> 00:01:23 Observatory in Hawaii, the biggest solar
00:01:23 --> 00:01:26 telescope ever built, a four metre mirror
00:01:26 --> 00:01:29 on Haleakala, zoomed in on the
00:01:29 --> 00:01:31 edges of the sun's granules. And where
00:01:31 --> 00:01:34 earlier telescopes saw a smooth, slightly
00:01:34 --> 00:01:37 blurry boundary, Inoue saw
00:01:37 --> 00:01:40 structure curling, breaking, wave
00:01:40 --> 00:01:42 like swirls forming and dissipating
00:01:42 --> 00:01:45 everywhere along the magnetic boundaries.
00:01:45 --> 00:01:47 Avery: And, um, these have a name. They're not a
00:01:47 --> 00:01:48 total surprise, physically.
00:01:48 --> 00:01:51 Anna: Right, exactly right. And that's what makes
00:01:51 --> 00:01:53 it satisfying rather than baffling. They're
00:01:53 --> 00:01:56 called Kelvin Helmholtz instabilities.
00:01:56 --> 00:01:59 If you've ever watched wind peel the top of
00:01:59 --> 00:02:02 an ocean wave, or seen those rows of curling
00:02:02 --> 00:02:04 cloud that look like a breaking sea in the
00:02:04 --> 00:02:07 sky, that's the same effect. It happens
00:02:07 --> 00:02:10 whenever two fluids slide past each other at
00:02:10 --> 00:02:13 different speeds. Lord Kelvin and Hermann
00:02:13 --> 00:02:15 Helmholtz described the math back around
00:02:15 --> 00:02:16 1870.
00:02:17 --> 00:02:20 Avery: So the physics is 150 years old. The
00:02:20 --> 00:02:22 picture of it on the sun's surface is four
00:02:22 --> 00:02:22 days old.
00:02:23 --> 00:02:26 Anna: That's the whole storey in one line. We've
00:02:26 --> 00:02:28 seen these swirls in Earth's clouds, in the
00:02:28 --> 00:02:31 atmospheres of Jupiter and Saturn, even
00:02:31 --> 00:02:33 hinted at high up in the sun's outer
00:02:33 --> 00:02:36 corona. But never before down on the
00:02:36 --> 00:02:39 visible surface, the Photosphere where the
00:02:39 --> 00:02:41 solar wind and all that magnetic energy
00:02:41 --> 00:02:44 actually originate. The resolution
00:02:44 --> 00:02:47 simply wasn't there. Inui changed that.
00:02:47 --> 00:02:49 Avery: Walk me through why the surface is the
00:02:49 --> 00:02:50 important place to catch them.
00:02:51 --> 00:02:53 Anna: Because that's where the sun's magnetic field
00:02:53 --> 00:02:56 tangles with its boiling convection. Picture
00:02:56 --> 00:02:59 the granules, those bright cells of hot
00:02:59 --> 00:03:02 plasma, rising, cooling, sinking
00:03:02 --> 00:03:05 like a pot of porridge on the boil at the
00:03:05 --> 00:03:08 edges. Flows crash into each other, and the
00:03:08 --> 00:03:10 magnetic field lines get squeezed together.
00:03:10 --> 00:03:13 Bundle field lines tighter, and the field
00:03:13 --> 00:03:16 gets stronger. The stronger field resists
00:03:16 --> 00:03:18 the plasma flow. And that sudden change in
00:03:18 --> 00:03:21 speed is exactly the shear you need to set a
00:03:21 --> 00:03:24 Kelvin Helmh vortex spinning.
00:03:24 --> 00:03:26 Avery: And they didn't just eyeball it and declare
00:03:26 --> 00:03:27 victory.
00:03:27 --> 00:03:30 Anna: No, this is the part I like. They ran the
00:03:30 --> 00:03:32 same magnetic region through a state of the
00:03:32 --> 00:03:35 art physics simulation, A model called
00:03:35 --> 00:03:38 Maram, built purely from the laws of
00:03:38 --> 00:03:41 physics. No fudging. And the simulated sun
00:03:41 --> 00:03:44 grew the same swirls in the same places with
00:03:44 --> 00:03:46 the same shapes. Observation and theory
00:03:47 --> 00:03:50 shaking hands. The Max Planck team called the
00:03:50 --> 00:03:52 agreement remarkable. And that's the word
00:03:52 --> 00:03:55 that earns this a, uh, nature paper. Not we
00:03:55 --> 00:03:58 saw something odd, but we saw it. We
00:03:58 --> 00:04:00 understand why. And the model agrees.
00:04:01 --> 00:04:03 Avery: So why should someone with feet firmly on the
00:04:03 --> 00:04:06 ground care about micro whirlpools
00:04:06 --> 00:04:07 93 million miles away?
00:04:08 --> 00:04:11 Anna: Two reasons, and they're both big. The
00:04:11 --> 00:04:13 first is one of the great unsolved puzzles in
00:04:13 --> 00:04:16 solar physics. The corona problem. The
00:04:16 --> 00:04:19 sun's surface is around 6 degrees.
00:04:20 --> 00:04:22 Its outer atmosphere, the corona, is
00:04:22 --> 00:04:25 millions of degrees, hundreds of times
00:04:25 --> 00:04:27 hotter. Further away from the heat source.
00:04:28 --> 00:04:30 That should be impossible. Like standing
00:04:30 --> 00:04:33 back from a campfire and getting warmer.
00:04:33 --> 00:04:36 Something is carrying energy upward and
00:04:36 --> 00:04:38 dumping it into the corona. And these
00:04:38 --> 00:04:41 ubiquitous little vortices are a very good
00:04:41 --> 00:04:43 candidate for part of that pipeline.
00:04:44 --> 00:04:46 Avery: And the second reason is the one that reaches
00:04:46 --> 00:04:49 down and touches U.S. base weather.
00:04:49 --> 00:04:52 Anna: Those same swirls could feed the buildup of
00:04:52 --> 00:04:54 magnetic energy that the sun eventually
00:04:54 --> 00:04:57 releases as flares and coronal mass
00:04:57 --> 00:04:59 ejections. The blasts of charged
00:04:59 --> 00:05:02 particles that, when they're aimed our way,
00:05:02 --> 00:05:05 can knock satellites about, degrade GPS
00:05:05 --> 00:05:08 and stress power grids. The next step
00:05:08 --> 00:05:10 is to turn pattern recognition algorithms
00:05:11 --> 00:05:13 loose on long runs of ENOYE data
00:05:13 --> 00:05:16 to measure how much these instabilities
00:05:16 --> 00:05:19 actually shift. Nail that number, and
00:05:19 --> 00:05:22 you sharpen the models that forecast solar
00:05:22 --> 00:05:22 storms.
00:05:23 --> 00:05:25 Avery: Which is a lovely place to be starting an
00:05:25 --> 00:05:26 eclipse week. Honestly, everyone's about to
00:05:26 --> 00:05:28 point their attention at the sun anyway.
00:05:29 --> 00:05:31 Anna: It really is. For decades, this was a
00:05:31 --> 00:05:34 prediction on a chalkboard. This week, it
00:05:34 --> 00:05:37 became a picture. The Sun's surface
00:05:37 --> 00:05:39 isn't a smooth glowing ball, it's a
00:05:39 --> 00:05:42 sea and it's full of breaking waves
00:05:43 --> 00:05:44 from the sun to
00:05:44 --> 00:05:46 Avery: the moon and to a storey. This show first
00:05:46 --> 00:05:48 flagged back in the autumn. Early Wednesday
00:05:48 --> 00:05:51 morning, a spent SpaceX Falcon 9 upper
00:05:51 --> 00:05:54 stage slammed into the far western edge of
00:05:54 --> 00:05:56 the moon near Einstein Crater at around half
00:05:56 --> 00:05:58 past two in the morning US Eastern time.
00:05:59 --> 00:06:01 Anna: This is the one astronomer Bill Grey had been
00:06:01 --> 00:06:02 tracking since April.
00:06:03 --> 00:06:05 Avery: The very one. Catalogue number
00:06:05 --> 00:06:08 2025 010D.
00:06:09 --> 00:06:11 Roughly four tonnes of hollow metal, about 12
00:06:11 --> 00:06:14 metres long. It launched in January last
00:06:14 --> 00:06:16 year, carrying two commercial lunar landers,
00:06:16 --> 00:06:19 Firefly's Blue Ghost and I. Space's
00:06:19 --> 00:06:21 resilience. Under NASA's Commercial Lunar
00:06:21 --> 00:06:23 Programme, its job done, it was left
00:06:23 --> 00:06:26 drifting. And for 19 months, sunlight
00:06:26 --> 00:06:29 and gravity nudged it around cislunar space
00:06:29 --> 00:06:31 until the numbers lined up on a collision
00:06:31 --> 00:06:32 course.
00:06:32 --> 00:06:35 Anna: And it hit at genuinely startling speed,
00:06:36 --> 00:06:38 Avery: about 5 miles an hour,
00:06:39 --> 00:06:41 seven times the speed of sound, releasing
00:06:41 --> 00:06:43 energy like roughly three tonnes of TNT.
00:06:44 --> 00:06:47 The catch for skywatchers, it came down on
00:06:47 --> 00:06:50 sunlit ground, so any flash was washed out by
00:06:50 --> 00:06:53 daylight. Nobody on Earth got the fireworks.
00:06:53 --> 00:06:56 Anna: So how do we actually confirm it happened
00:06:56 --> 00:06:59 and see the scar from orbit?
00:06:59 --> 00:07:01 Avery: And this is where it gets good. NASA's Lunar
00:07:01 --> 00:07:03 Reconnaissance Orbiter and South Korea's
00:07:03 --> 00:07:06 Dhanuri spacecraft are retasking to
00:07:06 --> 00:07:08 photograph the site. Because we know almost
00:07:08 --> 00:07:11 exactly where and when it struck. We get
00:07:11 --> 00:07:14 a rare before and after. A fresh crater
00:07:14 --> 00:07:16 expected somewhere between 18 and 30
00:07:16 --> 00:07:19 metres wide, appearing on a patch of moon we
00:07:19 --> 00:07:22 already had mapped. I'll be honest, those
00:07:22 --> 00:07:24 high resolution images aren't in hand yet.
00:07:24 --> 00:07:26 They depend on lighting and orbital geometry
00:07:26 --> 00:07:29 over the coming weeks. But the impact itself
00:07:29 --> 00:07:30 is confirmed.
00:07:30 --> 00:07:33 Anna: And there's a bigger point sitting underneath
00:07:33 --> 00:07:34 the spectacle.
00:07:34 --> 00:07:35 Avery: There is.
00:07:35 --> 00:07:37 This is only the second known unintentional
00:07:37 --> 00:07:40 lunar impact by a rocket stage. The first was
00:07:40 --> 00:07:43 a Chinese Booster back in 2022. But the
00:07:43 --> 00:07:46 traffic up there is climbing fast and there's
00:07:46 --> 00:07:48 still no binding rulebook for disposing of
00:07:48 --> 00:07:50 hardware on these high energy paths.
00:07:51 --> 00:07:53 SpaceX says this stage was passivated by the
00:07:53 --> 00:07:56 book and is now working with NASA on
00:07:56 --> 00:07:58 prevention. Fittingly, the international
00:07:58 --> 00:08:00 meeting that produced the latest
00:08:00 --> 00:08:02 recommendations for the moon was held right
00:08:02 --> 00:08:05 here in Sydney. The recommendations are real.
00:08:05 --> 00:08:07 The requirements aren't there yet.
00:08:07 --> 00:08:09 Anna: A new crater and a, uh, nudge to write some
00:08:09 --> 00:08:11 rules before the next one.
00:08:11 --> 00:08:14 Now to the most distant good news, Storey,
00:08:14 --> 00:08:17 you'll hear all year. Voyager 2, launched
00:08:17 --> 00:08:20 in 1977, now more than
00:08:20 --> 00:08:22 21 billion kilometres away out
00:08:22 --> 00:08:25 in Interstellar space has just been given
00:08:25 --> 00:08:28 at least another full year of science by
00:08:28 --> 00:08:31 engineers who can't touch it, can't send it
00:08:31 --> 00:08:33 apart and have to wait about 19 and a
00:08:33 --> 00:08:36 half hours just for a command to arrive.
00:08:37 --> 00:08:39 Avery: And they've given the manoeuvre a wonderful
00:08:39 --> 00:08:39 name.
00:08:39 --> 00:08:42 Anna: They're calling it the Big Bang. Here's the
00:08:42 --> 00:08:44 problem it Voyager runs on
00:08:44 --> 00:08:47 plutonium radioisotope generators
00:08:47 --> 00:08:50 that turn heat from decay into electricity
00:08:50 --> 00:08:53 and that supply drops by about 4
00:08:53 --> 00:08:55 watts every single year. It's a
00:08:55 --> 00:08:58 spacecraft slowly running out of power. And
00:08:58 --> 00:09:00 for years the fix has been to switch
00:09:00 --> 00:09:03 instruments off one by one without action.
00:09:03 --> 00:09:06 Voyager 2 would have had to shut down another
00:09:06 --> 00:09:09 of its three remaining instruments before the
00:09:09 --> 00:09:10 end of this year.
00:09:10 --> 00:09:13 Avery: So why Big Bang? What's dramatic about a
00:09:13 --> 00:09:14 power swap?
00:09:14 --> 00:09:17 Anna: Because it all had to happen at once. They
00:09:17 --> 00:09:19 switched off a set of power hungry devices
00:09:19 --> 00:09:22 and swapped in lower power alternatives.
00:09:22 --> 00:09:25 But the catch is that the very same power
00:09:25 --> 00:09:28 also produces heat. And out there, near
00:09:28 --> 00:09:31 absolute zero, if the wrong component gets
00:09:31 --> 00:09:33 too cold, it freezes and dies
00:09:33 --> 00:09:36 permanently. You can't do it gently, one
00:09:36 --> 00:09:39 step at a time. The thermal sums only
00:09:39 --> 00:09:41 balance if you throw the switches
00:09:41 --> 00:09:44 simultaneously. As one of the engineers put
00:09:44 --> 00:09:46 it, they couldn't afford to be wrong. And
00:09:46 --> 00:09:49 it worked exactly to plan.
00:09:49 --> 00:09:51 Avery: And Voyager 1 is next in the queue.
00:09:51 --> 00:09:54 Anna: It is. The team is stepping through the same
00:09:54 --> 00:09:57 process on Voyager 1 in the coming weeks. And
00:09:57 --> 00:10:00 the early tests have gone smoothly. Two
00:10:00 --> 00:10:02 probes, 48 years old, still
00:10:02 --> 00:10:05 humanity's only instruments physically out in
00:10:05 --> 00:10:08 interstellar space, kept alive by people
00:10:08 --> 00:10:11 rewriting how the hardware is used from
00:10:11 --> 00:10:14 13 billion miles back. That's not
00:10:14 --> 00:10:16 a rescue. That ends the storey. The power
00:10:16 --> 00:10:19 keeps falling. But it's another year of
00:10:19 --> 00:10:21 listening to the space between the stars.
00:10:21 --> 00:10:24 Avery: And now our, uh, running saga of the week.
00:10:24 --> 00:10:26 The rescue mission that spent the week being
00:10:26 --> 00:10:29 rescued. You'll remember the setup. NASA
00:10:29 --> 00:10:32 Swift Observatory, 22 years old, a
00:10:32 --> 00:10:34 first responder for gamma ray burst is
00:10:34 --> 00:10:37 sinking. Its orbit is decaying and it can't
00:10:37 --> 00:10:40 lift itself. And without help, it's likely to
00:10:40 --> 00:10:43 re enter this spring, our time. Once it drops
00:10:43 --> 00:10:44 below about 300 kilometres.
00:10:45 --> 00:10:48 Anna: Enter link. Built at extraordinary
00:10:48 --> 00:10:50 speed to go up and give Swift a boost.
00:10:50 --> 00:10:53 Avery: A commercial servicing spacecraft from
00:10:53 --> 00:10:55 Catalyst Space built clean sheet in about
00:10:55 --> 00:10:58 nine months. Launched last month. First of
00:10:58 --> 00:11:01 its kind. A private robot grabbing a
00:11:01 --> 00:11:03 government satellite that was never designed
00:11:03 --> 00:11:05 to be serviced, except that during
00:11:05 --> 00:11:08 commissioning, Link itself tumbled into a
00:11:08 --> 00:11:11 multi axis spin up to 9 degrees a
00:11:11 --> 00:11:13 second. With two of its three reaction wheels
00:11:13 --> 00:11:16 out of action and some loss in its cold gas
00:11:16 --> 00:11:19 thrusters. The rescuer needed a rescue.
00:11:19 --> 00:11:22 Anna: And this week is where that turned a corner.
00:11:22 --> 00:11:25 Avery: It genuinely did. Using thruster
00:11:25 --> 00:11:27 burns, the team has wrestled that spin all
00:11:27 --> 00:11:30 the way down from 9 degrees a second, uh, to
00:11:30 --> 00:11:32 1.47 degrees. And they're holding
00:11:32 --> 00:11:35 it steady there. The D spin effectively is
00:11:35 --> 00:11:38 one the mission has now shifted from a
00:11:38 --> 00:11:40 stabilisation problem to a software one.
00:11:41 --> 00:11:43 Because so much of the original attitude
00:11:43 --> 00:11:45 control system is offline, they're preparing
00:11:45 --> 00:11:48 a major flight software upgrade to restore
00:11:48 --> 00:11:50 full control using what still works.
00:11:51 --> 00:11:53 Anna: And only once that lands can the chase
00:11:53 --> 00:11:54 actually begin.
00:11:54 --> 00:11:57 Avery: Right, software update first, then the
00:11:57 --> 00:11:59 phasing manoeuvres to line Link's orbit up
00:11:59 --> 00:12:02 with Swift. Then a rendezvous and, uh, a
00:12:02 --> 00:12:05 grapple with its three robotic arms targeted
00:12:05 --> 00:12:07 around the end of August. If it all comes
00:12:07 --> 00:12:10 off, Lynx slowly walks Swift back up toward
00:12:10 --> 00:12:13 its old orbit over a couple of months, then
00:12:13 --> 00:12:16 peels away and burns up itself. It's down
00:12:16 --> 00:12:18 to the wire. But a week ago, this looked
00:12:18 --> 00:12:21 close to lost. And today it looks like a
00:12:21 --> 00:12:23 spacecraft catching its breath. Breath before
00:12:23 --> 00:12:24 the hardest part.
00:12:24 --> 00:12:26 Anna: We will absolutely keep you posted as that
00:12:26 --> 00:12:28 end of August window comes up.
00:12:28 --> 00:12:30 And so to the sky. And What a, uh, four days
00:12:30 --> 00:12:33 we're heading into. On Wednesday 12th
00:12:33 --> 00:12:36 August, two of the year's marquee events land
00:12:36 --> 00:12:39 together. A, uh, total solar eclipse and
00:12:39 --> 00:12:41 the peak of the Perseid meteor shower.
00:12:42 --> 00:12:44 Avery: Let's be straight with everyone about who
00:12:44 --> 00:12:47 sees what, because this one is lopsided.
00:12:47 --> 00:12:50 Anna: It is. So let's do it. Honestly, the
00:12:50 --> 00:12:53 total eclipse, the full daytime darkness,
00:12:53 --> 00:12:56 corona blazing spectacle, belongs to the
00:12:56 --> 00:12:59 far north. The path of totality crosses the
00:12:59 --> 00:13:01 Arctic, eastern Greenland, western Iceland
00:13:01 --> 00:13:04 and clips northern Spain and the very
00:13:04 --> 00:13:06 northeast of Portugal near sunset. If you're
00:13:06 --> 00:13:08 anywhere near there, you're in for one of the
00:13:08 --> 00:13:11 sky's greatest sights, under two and a half
00:13:11 --> 00:13:12 minutes of it.
00:13:12 --> 00:13:14 Avery: And, um, for our North American listeners,
00:13:14 --> 00:13:17 our largest audience, the honest picture is a
00:13:17 --> 00:13:19 partial and only in one corner.
00:13:20 --> 00:13:22 Anna: That's right. No part of North America sees
00:13:22 --> 00:13:25 totality this time. But in the afternoon on
00:13:25 --> 00:13:28 the 12th, Eastern Canada and the northeastern
00:13:28 --> 00:13:31 United States get a genuine partial in parts
00:13:31 --> 00:13:34 of Atlantic Canada, roughly half the sun
00:13:34 --> 00:13:36 covered at maximum. A smaller bite across New
00:13:36 --> 00:13:39 England and the Northeast further west, it
00:13:39 --> 00:13:42 fades to little or nothing. If you're in
00:13:42 --> 00:13:44 that eastern window, cheque local times for
00:13:44 --> 00:13:47 your exact town. It's an afternoon event. And
00:13:47 --> 00:13:49 dig out your eclipse glasses.
00:13:50 --> 00:13:51 Avery: Which brings us to the rule we
00:13:51 --> 00:13:54 Anna: never, ever skip the non
00:13:54 --> 00:13:57 negotiable. To look at any partial phase
00:13:57 --> 00:14:00 of the sun safely, you need proper solar
00:14:00 --> 00:14:01 filters. That meet the ISO
00:14:01 --> 00:14:04 123122 standard
00:14:05 --> 00:14:08 certified eclipse glasses or a safe solar
00:14:08 --> 00:14:11 viewer M ordinary sunglasses do not work
00:14:11 --> 00:14:13 no matter how dark. Only someone standing
00:14:13 --> 00:14:16 inside the path of totality may remove them
00:14:16 --> 00:14:18 and only during the brief total phase.
00:14:19 --> 00:14:21 Everyone seeing a partial, that's all of
00:14:21 --> 00:14:24 North America and most of Europe keeps them
00:14:24 --> 00:14:26 on the entire time. Damage to your eyes
00:14:26 --> 00:14:29 is painless and permanent. Please don't risk
00:14:29 --> 00:14:30 it.
00:14:30 --> 00:14:32 Avery: And if you're nowhere near the track, which
00:14:32 --> 00:14:34 includes all of us down here in the south,
00:14:34 --> 00:14:37 NASA streams the whole thing live from about
00:14:37 --> 00:14:38 a quarter past one eastern.
00:14:39 --> 00:14:42 Anna: Now the Perseids that same night and here the
00:14:42 --> 00:14:44 news is good for the northern half of the
00:14:44 --> 00:14:47 world. The peak lies the night of the 12th
00:14:47 --> 00:14:49 into the 13th and this year the peak is
00:14:49 --> 00:14:52 essentially moonless. The eclipse falls on a
00:14:52 --> 00:14:55 new moon so the sky is dark and the faint
00:14:55 --> 00:14:57 meteors get their moment from the mid
00:14:57 --> 00:15:00 northern latitudes after midnight that's
00:15:00 --> 00:15:02 potentially dozens an hour under clear skies.
00:15:02 --> 00:15:05 North America, Europe, this is your gift of
00:15:05 --> 00:15:06 the week.
00:15:06 --> 00:15:09 Avery: But the Perseids are a northern shower. The
00:15:09 --> 00:15:11 radiant barely lifts above the horizon.
00:15:11 --> 00:15:13 Anna: For those of us down here it barely clears
00:15:13 --> 00:15:16 it. So from Sydney or Auckland you'll catch
00:15:16 --> 00:15:19 only a stray few low in the north before
00:15:19 --> 00:15:21 dawn. So here's what the southern hemisphere
00:15:21 --> 00:15:24 actually gets and it's worth setting an alarm
00:15:24 --> 00:15:26 for before sunrise. This week the morning
00:15:26 --> 00:15:29 sky is stacked a long line of planets
00:15:29 --> 00:15:32 Saturn, Mars, Uranus and
00:15:32 --> 00:15:34 Neptunewith Jupiter low and Mercury
00:15:34 --> 00:15:37 climbing strung across the pre dawn.
00:15:37 --> 00:15:39 Venus is your brilliant evening star after
00:15:39 --> 00:15:42 sunset and for the patient Comet
00:15:42 --> 00:15:45 10P Tempel 2 is rising late in the
00:15:45 --> 00:15:48 evening around half past nine. If you've got
00:15:48 --> 00:15:49 binoculars and a dark
00:15:49 --> 00:15:52 Avery: horizon so nobody misses out. North gets
00:15:52 --> 00:15:54 the eclipse and the meteors. South gets the
00:15:54 --> 00:15:57 planet parade and a comet and the livestream
00:15:57 --> 00:15:58 is there for all of us.
00:15:58 --> 00:16:01 Anna: Both hemispheres eyes up all week, just
00:16:01 --> 00:16:03 protect them around that sun.
00:16:03 --> 00:16:06 Avery: That's the weekend wrap for Saturday 8th
00:16:06 --> 00:16:08 August. The Sun's hidden whirlpools, a
00:16:08 --> 00:16:11 fresh crater on the moon, Voyager 2's
00:16:11 --> 00:16:14 extra year and a rescue mission back on its
00:16:14 --> 00:16:14 feet.
00:16:14 --> 00:16:17 Anna: We're back with your daily fix on Monday and
00:16:17 --> 00:16:19 all week we'll be counting down to that
00:16:19 --> 00:16:22 eclipse and Perseid Wednesday. Find the full
00:16:22 --> 00:16:24 back catalogue, the news feed and the
00:16:24 --> 00:16:27 newsletter@uh astronomydailyio
00:16:27 --> 00:16:30 and say hello@astronomydailypod
00:16:30 --> 00:16:32 until Monday from Anna and me.
00:16:32 --> 00:16:35 Avery: Look after those eyes and clear skies.


