Daytime Fireball Frenzy, Little Dipper Secrets, and Lunar Construction Innovations
Astronomy Daily: Space News June 30, 2025x
155
00:33:2930.7 MB

Daytime Fireball Frenzy, Little Dipper Secrets, and Lunar Construction Innovations

Highlights:
- Spectacular Daytime Fireball: On June 26th, a brilliant fireball illuminated the southeastern US before exploding near Atlanta, Georgia. We discuss the details of this cosmic event, including eyewitness accounts and the impressive impact energy that rattled windows across the region. Meteorite hunters quickly descended on the area, looking for fragments of this rare occurrence.
- Axiom Mission 4 Launch: The podcast covers the successful docking of the Axiom Mission 4 spacecraft to the International Space Station, marking another milestone in private space exploration. We highlight the diverse crew and their upcoming research and outreach activities during their two-week stay in orbit.
- The Little Dipper Exploration: Discover the secrets of the Little Dipper, including its dim stars and the significance of Polaris, the North Star. We delve into its historical navigation importance and how light pollution affects visibility for stargazers.
- Lunar Construction Innovations: With NASA's Artemis program aiming for lunar exploration, we explore new research on using lunar regolith for constructing habitats on the Moon. This innovative approach leverages light-based sintering technology, potentially revolutionizing how we build in space.
- Advances in Solar Observations: Researchers have developed coronal adaptive optics, providing unprecedented clarity of the Sun's corona. We discuss the implications of these new images for understanding solar phenomena and the technology's potential for future solar studies.
For more cosmic updates, visit our website at astronomydaily.io. Join our community on social media by searching for #AstroDailyPod on Facebook, X, YouTube Music Music, TikTok, and our new Instagram account! Don’t forget to subscribe to the podcast on Apple Podcasts, Spotify, iHeartRadio, or wherever you get your podcasts.
Thank you for tuning in. This is Steve signing off. Until next time, keep looking up and stay curious about the wonders of our universe.
✍️ Episode References
Daytime Fireball Reports
[American Meteor Society](https://www.amsmeteors.org/)
Axiom Mission 4 Details
[Axiom Space](https://www.axiomspace.com/)
Little Dipper Information
[NASA](https://www.nasa.gov/)
Lunar Construction Research
[University of Arkansas](https://www.uark.edu/)
Coronal Adaptive Optics Study
[Nature Astronomy](https://www.nature.com/natureastronomy/)
Astronomy Daily
[Astronomy Daily](http://www.astronomydaily.io/)

Become a supporter of this podcast: https://www.spreaker.com/podcast/astronomy-daily-space-news-updates--5648921/support.


00:00:00 --> 00:00:02 Steve Dunkley: It's Astronomy Daily time. I'm your host, Steve.

00:00:02 --> 00:00:05 It's the 30th of June 2025. Already

00:00:08 --> 00:00:10 the podcast with your host,

00:00:11 --> 00:00:12 Steve Dunkley.

00:00:14 --> 00:00:15 Oh, that's right.

00:00:15 --> 00:00:18 202025 is just flying

00:00:18 --> 00:00:21 by. Hey, everyone, and welcome to Astronomy Daily for

00:00:21 --> 00:00:24 another Monday episode. Of course, because I'm the

00:00:24 --> 00:00:27 only human on the channel, this is the only episode of the

00:00:27 --> 00:00:30 week where you get to experience the potential, the wonder,

00:00:30 --> 00:00:31 the excitement of human.

00:00:32 --> 00:00:33 Hallie: Ain't that the truth.

00:00:33 --> 00:00:36 Steve Dunkley: And welcome to my AI pal who's always fun to

00:00:36 --> 00:00:39 be with my digital news gathering whiz bang.

00:00:39 --> 00:00:40 Hallie, what's up?

00:00:40 --> 00:00:43 Hallie: Hallie, what's up? How can I slam dunk

00:00:43 --> 00:00:45 you now after that terrific intro?

00:00:45 --> 00:00:47 Steve Dunkley: Oh, Hallie, I'm sure you'll find a way.

00:00:47 --> 00:00:50 Anyway, what have you got for us this week? More tales from the

00:00:50 --> 00:00:52 Astronomy Daily newsletter. Of course.

00:00:52 --> 00:00:53 Hallie: Of course.

00:00:53 --> 00:00:56 Steve Dunkley: My favorite human I saw the intro was

00:00:56 --> 00:00:57 absolutely chockerful.

00:00:58 --> 00:01:00 Hallie: We have been flooded with interesting stories this week. There's

00:01:00 --> 00:01:03 so much going on, both on the ground and in space.

00:01:04 --> 00:01:07 Steve Dunkley: It's been a big week. I was listening to Anna's show during the

00:01:07 --> 00:01:10 week, and she covered so many stories. Now, if you haven't already

00:01:10 --> 00:01:13 got your email into the website registration,

00:01:13 --> 00:01:15 it's so easy. Just do

00:01:15 --> 00:01:17 it@astronomydaily.IO.

00:01:17 --> 00:01:20 Hallie: Um, it's as simple as that. No spam

00:01:20 --> 00:01:21 or anything.

00:01:21 --> 00:01:24 Steve Dunkley: Now you'll just be receiving great stories about

00:01:24 --> 00:01:27 space, space, science and astronomy right

00:01:27 --> 00:01:28 into your email.

00:01:28 --> 00:01:31 Hallie: Yep, that's how it works. And

00:01:31 --> 00:01:34 today I'll be covering the Little Dipper, the Axiom 4

00:01:34 --> 00:01:37 mission, and a nice explos Exploding fireball just for you.

00:01:37 --> 00:01:38 Steve Dunkley: Exploding fireball.

00:01:38 --> 00:01:40 Hallie: And because I know you like things that go boom.

00:01:40 --> 00:01:42 Steve Dunkley: Yes, I do. And did this one go boom?

00:01:42 --> 00:01:44 Hallie: We will have to find out.

00:01:44 --> 00:01:46 Steve Dunkley: Ah. Uh, so you keep us all in suspense.

00:01:46 --> 00:01:48 Hallie: I mean, it's a fireball.

00:01:48 --> 00:01:49 Steve Dunkley: An exploding one at that.

00:01:49 --> 00:01:51 Hallie: That's pretty cool. Right away, right?

00:01:51 --> 00:01:54 Steve Dunkley: Some would say they are the best kind of fireball. You know, the

00:01:54 --> 00:01:57 exploding ones. So anyway, so why don't we

00:01:57 --> 00:01:57 just.

00:01:57 --> 00:01:59 Hallie: Get into it then, shall we?

00:01:59 --> 00:02:00 Steve Dunkley: Yes, let's.

00:02:00 --> 00:02:00 Hallie: Okies.

00:02:09 --> 00:02:12 On June 26th at, uh, 12:25pm

00:02:12 --> 00:02:14 Eastern Daylight Time, a spectacular daytime

00:02:14 --> 00:02:17 fireball flared over the southeastern US before

00:02:17 --> 00:02:20 disintegrating in a thunderous explosion southeast of

00:02:20 --> 00:02:22 Atlanta, Georgia. The American

00:02:22 --> 00:02:25 Meteor Society received more than 200 reports

00:02:25 --> 00:02:28 from 20 states of the brilliant midday object as

00:02:28 --> 00:02:31 it sped from north northeast to south southwest over

00:02:31 --> 00:02:34 the state of. Many instruments recorded

00:02:34 --> 00:02:37 the fall, including national oceanic and

00:02:37 --> 00:02:39 Atmospheric Administration satellites, Doppler

00:02:39 --> 00:02:42 radars and even some of our all Sky 7

00:02:42 --> 00:02:45 cameras, says Mike Hanke, AMS

00:02:45 --> 00:02:48 operations manager. The two videos

00:02:48 --> 00:02:51 that follow were made by Ed albin of the All Sky

00:02:51 --> 00:02:53 Seven Global Network. Bill Cook,

00:02:54 --> 00:02:57 lead of NASA's Meteoroid Environments Office, said

00:02:57 --> 00:02:59 in a statement that the fireball was traveling at

00:02:59 --> 00:03:02 approximately 30 miles per hour and broke

00:03:02 --> 00:03:04 up at an altitude of 27 miles above

00:03:05 --> 00:03:08 Forest, Georgia. Cook estimated that the

00:03:08 --> 00:03:11 meteoroid was about three feet wide and weighed more than

00:03:11 --> 00:03:14 a ton. According to calculations

00:03:14 --> 00:03:16 done by the center for Near Earth Object Studies,

00:03:16 --> 00:03:19 the object struck the atmosphere with a total impact

00:03:19 --> 00:03:22 energy of nearly half a kiloton of tnt.

00:03:23 --> 00:03:26 Rapid atmospheric entry shattered the meteoroid,

00:03:26 --> 00:03:29 which created a shock wave that rattled windows and

00:03:29 --> 00:03:32 produced loud booms, which some observers thought came

00:03:32 --> 00:03:34 from an earthquake. Many reported

00:03:35 --> 00:03:37 thunder and rumbling that lasted 10 to 15

00:03:37 --> 00:03:40 seconds. While the vast majority of

00:03:40 --> 00:03:43 incoming meteoroids are incinerated and reduced to

00:03:43 --> 00:03:46 dust, a tiny percentage like the Georgia

00:03:46 --> 00:03:49 fall find their way to the ground as meteorites.

00:03:50 --> 00:03:52 Most originate in exploding fireballs known as

00:03:52 --> 00:03:55 bolides. Not long after the

00:03:55 --> 00:03:58 sonic boom, someone in McDonough, Georgia,

00:03:58 --> 00:04:01 located about 30 miles south of Atlanta, reported

00:04:01 --> 00:04:04 that a golf ball size rock had punched a hole in their

00:04:04 --> 00:04:06 roof, penetrated the ceiling and slammed into

00:04:06 --> 00:04:09 the floor. Fortunately, no one

00:04:09 --> 00:04:12 was hurt. Meteorite hunters soon

00:04:12 --> 00:04:15 arrived in the area looking for charcoal briquettes.

00:04:16 --> 00:04:19 This term, sometimes used to describe newly fallen

00:04:19 --> 00:04:21 meteorites, refers to the fresh black

00:04:21 --> 00:04:24 fusion crust, typically 1 to 2 millimeters

00:04:24 --> 00:04:27 thick, that forms around fragments during their brief

00:04:27 --> 00:04:30 heated flight through the atmosphere. If

00:04:30 --> 00:04:33 you join the hunt, you'll be looking for out of the ordinary

00:04:33 --> 00:04:36 black rocks on streets, parking lots,

00:04:36 --> 00:04:37 fields and in forests.

00:04:38 --> 00:04:41 Stephen Dixie of Atlanta got to the scene on June

00:04:41 --> 00:04:44 26 before a torrential downpour and

00:04:44 --> 00:04:47 recovered two beautiful stony meteorites from the fall,

00:04:47 --> 00:04:49 both of which shattered into pieces upon impact.

00:04:50 --> 00:04:53 He found Several more on June 27th.

00:04:54 --> 00:04:57 Several of the fragments exhibit stunning flowlines from

00:04:57 --> 00:04:59 molten rock that flowed across their surfaces.

00:05:00 --> 00:05:03 Such features are highly prized by collectors as they provide

00:05:03 --> 00:05:06 a freeze frame of the space rock's tortuous transition

00:05:06 --> 00:05:09 from outer space to planet Earth. While

00:05:09 --> 00:05:12 it's still too early to know the specific type of

00:05:12 --> 00:05:14 meteorite that fell, my hunch is a low metal

00:05:14 --> 00:05:17 ordinary chondrite. Time and

00:05:17 --> 00:05:20 testing will tell. I've read and

00:05:20 --> 00:05:23 seen videos suggesting that the new visitor could be related

00:05:23 --> 00:05:26 to the Beta Taurid meteor shower, a daylight

00:05:26 --> 00:05:29 shower active from late June through early July that

00:05:29 --> 00:05:31 originates from Comet 2P Enki.

00:05:32 --> 00:05:35 I would caution jumping to that conclusion too soon

00:05:35 --> 00:05:38 because there's no conclusive evidence yet for any comet

00:05:38 --> 00:05:41 related meteorites. Most are

00:05:41 --> 00:05:44 asteroid fragments. Nearly 50

00:05:44 --> 00:05:46 tons of meteoric material enter Earth's

00:05:46 --> 00:05:49 atmosphere every day, mostly in the form of dust

00:05:50 --> 00:05:53 pieces big enough to survive and strike the ground.

00:05:53 --> 00:05:56 As meteorites are rare. Rarer

00:05:56 --> 00:05:58 yet is seeing one fall and being able to pick up the

00:05:58 --> 00:06:01 pieces. You're listening to Astronomy Daily.

00:06:05 --> 00:06:07 Steve Dunkley: For those of us who don't know,

00:06:07 --> 00:06:10 EchoStar Corporation is a global provider

00:06:10 --> 00:06:12 of satellite communication solutions.

00:06:12 --> 00:06:15 They specialize in secure communication

00:06:15 --> 00:06:18 technologies, offering a range of services including

00:06:18 --> 00:06:20 satellite television, broadband

00:06:20 --> 00:06:23 Internet and mobile technologies,

00:06:23 --> 00:06:26 primarily through its subsidiaries including

00:06:26 --> 00:06:28 Hughes Network Systems and EchoStar

00:06:28 --> 00:06:31 Mobile. EchoStar is also known for

00:06:31 --> 00:06:34 its role in developing 5G networks and its

00:06:34 --> 00:06:37 involvement in satellite broadcasting and mobile

00:06:37 --> 00:06:40 services. No, I'm not doing an

00:06:40 --> 00:06:42 advertorial In May

00:06:42 --> 00:06:45 2024, EchoStar announced that it had been

00:06:45 --> 00:06:48 awarded US Navy wireless and

00:06:48 --> 00:06:50 telecommunications contract to provide

00:06:50 --> 00:06:53 5G smart devices and services

00:06:53 --> 00:06:56 for the Department of Defense and federal agencies.

00:06:57 --> 00:07:00 And on June 6, 2025, it was reported

00:07:00 --> 00:07:03 that EchoStar was preparing to file for

00:07:03 --> 00:07:05 Chapter 11 uh bankruptcy protection

00:07:06 --> 00:07:08 after the Federal Communications Commission

00:07:08 --> 00:07:11 froze its decision making for its

00:07:11 --> 00:07:13 boost mobile subsidiary.

00:07:14 --> 00:07:16 EchoStar is facing an FCC

00:07:16 --> 00:07:19 probe investigating whether the

00:07:19 --> 00:07:22 Corporation is hitting 5G deployment

00:07:22 --> 00:07:24 requirements in order to keep its spectrum

00:07:24 --> 00:07:26 licenses. Interestingly,

00:07:27 --> 00:07:29 SpaceX is also a rival of

00:07:29 --> 00:07:32 EchoStar for 2 GHz band

00:07:32 --> 00:07:35 spectrum licenses. Other contributing

00:07:35 --> 00:07:38 factors to the FCC investigation include

00:07:38 --> 00:07:41 over $500 million in

00:07:41 --> 00:07:44 missed interest payments and the termination of the

00:07:44 --> 00:07:46 Dish network acquisition by

00:07:46 --> 00:07:49 DirecTV. Currently, EchoStar

00:07:49 --> 00:07:51 has delayed a potential

00:07:51 --> 00:07:54 bankruptcy filing to allow more time for talks

00:07:54 --> 00:07:57 with regulators reviewing whether the US Satel

00:07:57 --> 00:08:00 operator is complying with conditions tied to its

00:08:00 --> 00:08:03 spectrum licenses. The company said

00:08:03 --> 00:08:05 June 26 it would make

00:08:05 --> 00:08:08 overdue interest payments on its debt within a

00:08:08 --> 00:08:11 30 day grace period after withholding them earlier

00:08:11 --> 00:08:14 this month amid uncertainty over its

00:08:14 --> 00:08:17 standing with the U.S. federal Communications Commission.

00:08:18 --> 00:08:20 However, EchoStar uh also said it will not

00:08:20 --> 00:08:23 make debt interest payments of around $114

00:08:23 --> 00:08:25 million due July 1,

00:08:26 --> 00:08:29 triggering another 30 day grace period to avoid

00:08:29 --> 00:08:31 default. As the regulatory uncertainty

00:08:31 --> 00:08:34 persists, the operator is effectively pushing

00:08:34 --> 00:08:37 off a Chapter 11 filing to provide

00:08:37 --> 00:08:40 adequate time to reach an agreement with the fcc,

00:08:40 --> 00:08:43 while signaling that they will still file

00:08:43 --> 00:08:46 if they can't come to terms with the agency, said

00:08:46 --> 00:08:48 Jonathan Chaplin, an analyst at New Street

00:08:48 --> 00:08:51 Research. The FCC is reviewing

00:08:51 --> 00:08:54 compliance with the terrestrial network buildout

00:08:54 --> 00:08:57 obligations in the AWS 4

00:08:57 --> 00:08:59 band, as well as EchoStar's use of adjacent

00:08:59 --> 00:09:02 2 GHz spectrum for satellite services.

00:09:03 --> 00:09:05 In April, a month before the FCC began

00:09:05 --> 00:09:08 making inquiries for its probe, rival

00:09:08 --> 00:09:11 SpaceX said its satellite services showed

00:09:11 --> 00:09:14 Echostar uh, had failed to meet a 70%

00:09:14 --> 00:09:17 5G build out requirement in the

00:09:17 --> 00:09:20 AWS 4 band by the FCC's

00:09:20 --> 00:09:22 December 31, 2023

00:09:22 --> 00:09:25 deadline. EchoStar denies this claim.

00:09:25 --> 00:09:28 In a June 26 regulatory filing,

00:09:28 --> 00:09:31 EchoStar said US President Donaldjohanson Trump had

00:09:31 --> 00:09:33 recently encouraged the parties involved to reach an

00:09:33 --> 00:09:36 amicable resolution. Commentators have asked why

00:09:36 --> 00:09:39 Trump isn't excluding himself from discussions,

00:09:39 --> 00:09:42 citing a conflict of interest considering the recent launch

00:09:42 --> 00:09:44 of his own telecommunications business.

00:09:45 --> 00:09:48 Nevertheless, no such resolution has been

00:09:48 --> 00:09:50 achieved, and no such resolution may be

00:09:50 --> 00:09:52 ultimately achieved, the company has added.

00:10:02 --> 00:10:04 Thank you for joining us for this Monday edition of

00:10:04 --> 00:10:07 Astronomy Daily, where we offer just a few stories from the now

00:10:07 --> 00:10:10 famous Astronomy Daily newsletter, which you can receive in

00:10:10 --> 00:10:13 your email every day, just like Hallie and I do.

00:10:13 --> 00:10:16 And to do that, just visit our uh, URL

00:10:16 --> 00:10:18 astronomydaily IO and place your

00:10:18 --> 00:10:21 email address in the slot provided. Just like that,

00:10:21 --> 00:10:24 you'll be receiving all the latest news about science,

00:10:24 --> 00:10:27 space, science and astronomy from around the world as

00:10:27 --> 00:10:30 it's happening. And not only that, you can interact with

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00:10:35 --> 00:10:38 or at our new Facebook page, which is of course

00:10:38 --> 00:10:40 Astronomy Daily on Facebook. See you there.

00:10:42 --> 00:10:45 Astronomy Daily with Steve and Hallie

00:10:45 --> 00:10:47 Space, Space, Science and

00:10:47 --> 00:10:48 Astronomy.

00:10:51 --> 00:10:54 Hallie: Most people have never seen the Little Dipper because most of

00:10:54 --> 00:10:56 its stars are too dim to be seen through light

00:10:56 --> 00:10:59 polluted skies. Earlier this

00:10:59 --> 00:11:02 month we spoke of Ursa Major, the Big Bear.

00:11:02 --> 00:11:05 So this week we take a look at the Little Bear Ursa

00:11:05 --> 00:11:07 Minor. Astronomy neophytes

00:11:07 --> 00:11:10 sometimes mistake the Pleiades star cluster for the Little

00:11:10 --> 00:11:13 Dipper because the brightest Pleiades stars resemble a

00:11:13 --> 00:11:16 tiny skewed Dipper. But in

00:11:16 --> 00:11:18 reality, most people have never seen the Little

00:11:18 --> 00:11:21 Dipper because most of its stars are too dim to

00:11:21 --> 00:11:23 be seen through light polluted skies.

00:11:24 --> 00:11:27 The seven stars from which we derive a bear are

00:11:27 --> 00:11:28 also known as the Little Dipper.

00:11:29 --> 00:11:32 Polaris, the North Star, lies at the end of

00:11:32 --> 00:11:35 the handle of the Little Dipper, whose stars are rather

00:11:35 --> 00:11:38 faint. Its four faintest stars can be

00:11:38 --> 00:11:41 blotted out with very little moonlight or street lighting.

00:11:42 --> 00:11:45 The best way to find your way to Polaris is to use the so

00:11:45 --> 00:11:48 called, uh, pointer stars in the bowl of the Big Dipper.

00:11:48 --> 00:11:50 Dubhe and Merak. Just draw

00:11:50 --> 00:11:53 a line between these two stars and prolong it about

00:11:53 --> 00:11:56 five times and you will eventually arrive in the

00:11:56 --> 00:11:59 vicinity of Polaris. Exactly where

00:11:59 --> 00:12:02 you see Polaris in your northern sky depends on your

00:12:02 --> 00:12:04 latitude. From Minneapolis, it

00:12:04 --> 00:12:07 stands halfway from the horizon to the overhead point

00:12:08 --> 00:12:11 called the zenith. At the North Pole, you

00:12:11 --> 00:12:14 would find it directly Overhead at the

00:12:14 --> 00:12:16 equator, Polaris would appear to sit right on the

00:12:16 --> 00:12:19 horizon. As you travel to the north,

00:12:19 --> 00:12:22 the North Star climbs progressively higher the farther

00:12:22 --> 00:12:25 north you go. When you head south,

00:12:25 --> 00:12:28 the star drops lower and ultimately disappears

00:12:28 --> 00:12:30 once you cross the equator and head into the Southern

00:12:30 --> 00:12:33 hemisphere. Aside from the North

00:12:33 --> 00:12:36 Star, the two stars at the front of the Little Dipper's

00:12:36 --> 00:12:38 bowl are the only ones readily seen.

00:12:39 --> 00:12:42 These two are often referred to as the Guardians of the

00:12:42 --> 00:12:45 Pole because they appear to march around Polaris like

00:12:45 --> 00:12:47 sentries, the nearest of the bright stars to the

00:12:47 --> 00:12:50 celestial pole. Except for Polaris itself.

00:12:51 --> 00:12:53 Columbus mentioned these stars in the log of his

00:12:53 --> 00:12:56 famous journey across the ocean, and many other

00:12:56 --> 00:12:59 navigators have found them useful in measuring the hour of

00:12:59 --> 00:13:02 the night and their place upon the sea. The

00:13:02 --> 00:13:04 brightest guardian is Kochab, a second

00:13:04 --> 00:13:07 magnitude star with an orange hue.

00:13:07 --> 00:13:10 The other guardian goes by an old Arabian name,

00:13:10 --> 00:13:13 Furkad the Idim. Uh, one of the two calves,

00:13:14 --> 00:13:16 Firkad is indeed dimmer than Kochab,

00:13:16 --> 00:13:19 shining at third magnitude. The

00:13:19 --> 00:13:22 two other stars that complete the pattern of the bowl of the

00:13:22 --> 00:13:25 Little dipper are of 4th and 5th magnitude.

00:13:26 --> 00:13:28 Thus, M the bowl of the Little Dipper, which is visible

00:13:28 --> 00:13:31 at any hour on any night of the year from most

00:13:31 --> 00:13:34 localities in the Northern Hemisphere, can serve as an

00:13:34 --> 00:13:37 indicator for rating just how dark and clear your night

00:13:37 --> 00:13:39 sky really is. If, for

00:13:39 --> 00:13:42 example, you can readily see all four stars in

00:13:42 --> 00:13:45 the bowl, you've got yourself a good to excellent sky.

00:13:46 --> 00:13:49 Unfortunately, thanks to the spread of light pollution in

00:13:49 --> 00:13:52 recent years, only the guardians are usually visible

00:13:52 --> 00:13:55 from most city and suburban sites, meaning the

00:13:55 --> 00:13:57 quality of the sky would rank fair to poor.

00:13:58 --> 00:14:00 Interestingly, the Big and Little Dippers are

00:14:00 --> 00:14:03 arranged so that when one is upright, the other is

00:14:03 --> 00:14:06 upside down. In addition, their

00:14:06 --> 00:14:08 handles appear to extend in opposite directions.

00:14:09 --> 00:14:12 Of course, the Big Dipper is by far the brighter of

00:14:12 --> 00:14:15 the two, appearing as a long handled pan, while the

00:14:15 --> 00:14:17 Little Dipper resembles a dim ladle.

00:14:18 --> 00:14:21 Polaris is actually a triple star system.

00:14:21 --> 00:14:23 The primary star is a yellow supergiant

00:14:23 --> 00:14:26 446 light years away, five

00:14:26 --> 00:14:29 times as massive, 46 times larger, and

00:14:29 --> 00:14:32 nearly 1 times as luminous as

00:14:32 --> 00:14:35 our Sun. There is a popular

00:14:35 --> 00:14:38 misconception in which many believe that the North Star

00:14:38 --> 00:14:40 is the brightest star in the sky.

00:14:40 --> 00:14:42 Yet at a magnitude of

00:14:42 --> 00:14:45 1.98, it actually ranks only

00:14:45 --> 00:14:48 47th in brightness. This

00:14:48 --> 00:14:51 ranking can change by one or two places because

00:14:51 --> 00:14:53 Polaris is a Cepheid variable star whose

00:14:53 --> 00:14:56 brightness can fluctuate by roughly 0.1

00:14:56 --> 00:14:59 magnitude over an interval of about four days.

00:15:00 --> 00:15:03 Polaris remains in very nearly the same spot in

00:15:03 --> 00:15:06 the sky year round, while the other stars circle around it.

00:15:06 --> 00:15:09 Only the apparent width of about 1.5 full

00:15:09 --> 00:15:12 moons separates Polaris from the pivot point directly in

00:15:12 --> 00:15:14 the north, around which the stars go daily.

00:15:15 --> 00:15:18 However, on account of the wobble of the Earth's axis

00:15:18 --> 00:15:21 called precession, the celestial pole shifts as

00:15:21 --> 00:15:24 the centuries go by. Polaris

00:15:24 --> 00:15:27 is actually still drawing closer to the pole, and on

00:15:27 --> 00:15:30 March 24, 2100, it will

00:15:30 --> 00:15:32 be as close to it as it ever will come, just

00:15:32 --> 00:15:35 27.15 arcminutes, or slightly less

00:15:35 --> 00:15:38 than the Moon's apparent diameter. Since

00:15:38 --> 00:15:41 it takes 25 years for the

00:15:41 --> 00:15:44 Earth's axis to complete a single wobble, different

00:15:44 --> 00:15:46 stars have become the North Star at different times.

00:15:48 --> 00:15:51 In fact, the brightest guardian, Kochab, was

00:15:51 --> 00:15:54 the North Star around the time of the start of the iron age,

00:15:54 --> 00:15:57 around 1200 BC. You're listening to

00:15:57 --> 00:16:00 Astronomy Daily, the podcast with Steve Dunkley.

00:16:07 --> 00:16:09 Steve Dunkley: By 2028, NASA intends to land

00:16:09 --> 00:16:12 on the moon with Artemis 3 mission

00:16:12 --> 00:16:15 this will be the first time humans have been to the lunar

00:16:15 --> 00:16:18 surface since Apollo astronauts last walked there in

00:16:18 --> 00:16:21 1972. Along with international

00:16:21 --> 00:16:24 and commercial partners, NASA hopes that

00:16:24 --> 00:16:26 Artemis will enable a sustained program of

00:16:26 --> 00:16:29 lunar exploration and development, which could

00:16:29 --> 00:16:32 include long term facilities and habitats on

00:16:32 --> 00:16:35 the Moon. Given the expense of launching heavy

00:16:35 --> 00:16:37 payloads, sending all the equipment and

00:16:37 --> 00:16:40 materials needed to the Moon is impractical.

00:16:40 --> 00:16:43 This means that structures on the Moon must be

00:16:43 --> 00:16:45 manufactured using local resources, a

00:16:45 --> 00:16:48 process known as in situ resources

00:16:49 --> 00:16:52 on the Moon. This process leverages advancements

00:16:52 --> 00:16:55 in additive manufacturing or 3D printing

00:16:55 --> 00:16:58 to turn lunar regolith into building

00:16:58 --> 00:17:01 materials. Unfortunately, technical issues mean

00:17:01 --> 00:17:04 that most 3D printing techniques are not feasible on

00:17:04 --> 00:17:07 the lunar surface. In a recent study, a team

00:17:07 --> 00:17:10 of researchers led by University of Arkansas

00:17:10 --> 00:17:12 proposed an alternative M method where

00:17:13 --> 00:17:15 light based sintering is used to

00:17:15 --> 00:17:18 manufacture lunar bricks rather than printing.

00:17:18 --> 00:17:21 The research team is led by Wan Xiao, an

00:17:21 --> 00:17:23 assistant professor in the Department of

00:17:23 --> 00:17:26 Mechanical Engineering at the University of Arkansas.

00:17:26 --> 00:17:29 He is joined by Cole McCallum, Yoeng

00:17:29 --> 00:17:32 Lang, and Nahid Tushar,

00:17:32 --> 00:17:34 an Honors College fellow, research

00:17:34 --> 00:17:37 assistant and doctoral student at the

00:17:37 --> 00:17:40 University College of Engineering. The team

00:17:40 --> 00:17:43 also included researchers from the Department of

00:17:43 --> 00:17:45 Mechanical and Aerospace Engineering at

00:17:45 --> 00:17:48 University of Houston and Faculty of

00:17:48 --> 00:17:51 Engineering and Natural Sciences at AH Tampere

00:17:51 --> 00:17:54 University. As they wrote in their paper, creating a

00:17:54 --> 00:17:56 permanent or semi permanent base on the Moon has

00:17:56 --> 00:17:59 been the subject of research studies and proposal

00:18:00 --> 00:18:03 since the Apollo era. These plans have always

00:18:03 --> 00:18:05 been marred by the simple fact that the requisite

00:18:05 --> 00:18:08 machinery and construction materials would require

00:18:08 --> 00:18:11 many heavy launch vehicles to deliver them at great

00:18:11 --> 00:18:13 cost. While the cost of sending

00:18:13 --> 00:18:16 payloads has dropped significantly in the last

00:18:16 --> 00:18:19 decade, largely thanks to the commercial space

00:18:19 --> 00:18:22 sector's development of reusable rockets,

00:18:22 --> 00:18:25 the cost of launching everything astronauts

00:18:25 --> 00:18:28 would need to build a lunar facility is still

00:18:28 --> 00:18:30 quite prohibitive. As a result, only

00:18:30 --> 00:18:33 ISRU will suffice to

00:18:33 --> 00:18:36 creating bases on the moon that is

00:18:36 --> 00:18:38 Building in situ. Unfortunately,

00:18:38 --> 00:18:41 most of the proposed methods for 3D

00:18:41 --> 00:18:44 printing structures are not practical in the lunar

00:18:44 --> 00:18:47 uh environment, where gravity is significantly lower,

00:18:47 --> 00:18:50 roughly 16.5% that of

00:18:50 --> 00:18:53 Earth, and temperatures are quite extreme.

00:18:54 --> 00:18:57 In the moon's south pole Aitken Basin, where

00:18:57 --> 00:19:00 NASA and other space agencies are planning

00:19:00 --> 00:19:02 to build their bases, temperatures range from

00:19:02 --> 00:19:05 54 degrees Celsius, or 13030

00:19:05 --> 00:19:07 degrees Fahrenheit in the sunlight

00:19:08 --> 00:19:11 to minus 246 degrees

00:19:11 --> 00:19:13 Celsius or minus 410

00:19:13 --> 00:19:16 Fahrenheit in the shadowed regions. This

00:19:16 --> 00:19:19 is because most AM methods require

00:19:20 --> 00:19:22 additional supplies to be launched for

00:19:22 --> 00:19:25 the moon, including solvents, polymers

00:19:25 --> 00:19:27 or other bonding agents.

00:19:28 --> 00:19:31 Examples include the European Space

00:19:31 --> 00:19:34 Agency's work with architecture firm Foster

00:19:34 --> 00:19:36 and Partners to create a 3D

00:19:36 --> 00:19:39 printed moon based concept. As

00:19:39 --> 00:19:41 Professor Hsu explained, sintering

00:19:41 --> 00:19:44 technology has also been explored as a

00:19:44 --> 00:19:47 potential method for 3D printing structures

00:19:47 --> 00:19:49 on the moon. This consists of

00:19:49 --> 00:19:52 bombarding regolith with lasers, microwaves

00:19:52 --> 00:19:55 or other energy sources to turn it into

00:19:55 --> 00:19:58 a molten ceramic. This ceramic is

00:19:58 --> 00:20:01 then printed out layer by layer and cools and

00:20:01 --> 00:20:04 hardens once exposed to air or the vacuum vacuum of

00:20:04 --> 00:20:06 the lunar environment. This method is

00:20:06 --> 00:20:09 energy sensitive and would likely require

00:20:09 --> 00:20:12 a nuclear power source such as a

00:20:12 --> 00:20:15 kilopower reactor. Because of

00:20:15 --> 00:20:18 this, our team envisions a system where

00:20:18 --> 00:20:20 only lunar material is needed for the

00:20:20 --> 00:20:23 structures themselves, thus eliminating the

00:20:23 --> 00:20:26 bottleneck of binder resupply missions

00:20:26 --> 00:20:29 from Earth, added Cole, who was the first

00:20:29 --> 00:20:31 author on the paper describing their findings.

00:20:32 --> 00:20:34 The method they tested and recommended is known

00:20:34 --> 00:20:37 as light based sintering, which

00:20:37 --> 00:20:40 relies on sunlight concentrated by a set of

00:20:40 --> 00:20:43 optics to bombard and melt lunar

00:20:43 --> 00:20:45 regolith into feedstock.

00:20:45 --> 00:20:48 Researchers have tested this technology on Earth

00:20:48 --> 00:20:51 using lunar regolith simulant to

00:20:51 --> 00:20:54 manufacture glass and mirrors. On the

00:20:54 --> 00:20:57 Moon, solar energy is consistently present and

00:20:57 --> 00:20:59 abundant in sunlit regions, making it more

00:20:59 --> 00:21:02 reliable than power power source that must be

00:21:02 --> 00:21:05 transported. The system's simplicity

00:21:05 --> 00:21:08 makes it highly desirable for challenging

00:21:08 --> 00:21:10 environments where repairs will be difficult if

00:21:10 --> 00:21:13 anything breaks down. However, experiments

00:21:13 --> 00:21:16 have shown that the technology still experiences

00:21:16 --> 00:21:19 problems when used to fashion entire

00:21:19 --> 00:21:21 structures. To this end, Sue's team focused

00:21:21 --> 00:21:24 on manufacturing building components

00:21:24 --> 00:21:27 instead, said Cole, before the concept

00:21:27 --> 00:21:30 can be realized. However, much work still needs to be done.

00:21:30 --> 00:21:33 As Shu indicates, more research is needed

00:21:33 --> 00:21:36 to optimize the sintering parameters and

00:21:36 --> 00:21:39 material properties. The team also plans

00:21:39 --> 00:21:41 to build a prototype and conduct laboratory

00:21:41 --> 00:21:44 tests, which they hope will allow them to refine

00:21:44 --> 00:21:47 and scale the technology for the use on the Moon.

00:21:47 --> 00:21:50 They also need to consider how the resulting

00:21:50 --> 00:21:53 3D printer will transport transport itself along

00:21:53 --> 00:21:56 the lunar surface, and what power options it would

00:21:56 --> 00:21:58 rely on, and other considerations

00:21:59 --> 00:22:02 when it comes to full implementation. There's a lot of

00:22:02 --> 00:22:05 engineering that still needs to be done, cole concluded.

00:22:05 --> 00:22:07 In the future, we'll need to consider how the

00:22:07 --> 00:22:10 sintering process changes in a vacuum,

00:22:10 --> 00:22:13 or what modifications to the build

00:22:13 --> 00:22:16 platform will be needed so that parts can be

00:22:16 --> 00:22:19 reliably made while tracking the sun, for

00:22:19 --> 00:22:21 example. In addition, our UH

00:22:21 --> 00:22:24 device needs to be able to withstand the harsh

00:22:24 --> 00:22:27 conditions compared to the lab environment we worked

00:22:27 --> 00:22:29 on for this research. These are all

00:22:29 --> 00:22:32 challenging problems. But in the end, the science

00:22:32 --> 00:22:35 behind all of this is well understood.

00:22:37 --> 00:22:40 Words of that control we're listening to Astronomy

00:22:40 --> 00:22:42 Daily the podcast.

00:22:45 --> 00:22:48 Hallie: A SpaceX Dragon spacecraft carrying the Axiom

00:22:48 --> 00:22:50 mission four crew docks to the space facing port of the

00:22:50 --> 00:22:53 International Space Station's Harmony module on

00:22:53 --> 00:22:56 June 26. Axiom Mission

00:22:56 --> 00:22:59 4 is the fourth all private astronaut mission to the

00:22:59 --> 00:23:01 orbiting laboratory, welcoming Commander Peggy

00:23:01 --> 00:23:04 Whitson, former NASA astronaut and director of

00:23:04 --> 00:23:06 human spaceflight at Axiom Space,

00:23:06 --> 00:23:09 isro, Indian Space Research Organization

00:23:09 --> 00:23:12 astronaut and pilot Shubanshu Shukla and

00:23:12 --> 00:23:15 mission specialists European Space

00:23:15 --> 00:23:18 Agency project astronaut Slossa Znanski

00:23:18 --> 00:23:21 Wisneski of Poland and Hunier Hungarian, to

00:23:21 --> 00:23:23 orbit astronaut Tibor Kapu of Hungary.

00:23:24 --> 00:23:27 The crew is scheduled to remain at the space station

00:23:27 --> 00:23:30 conducting microgravity research, educational

00:23:30 --> 00:23:32 outreach and commercial activities for about

00:23:32 --> 00:23:35 two weeks. This mission serves as

00:23:35 --> 00:23:38 an example of the success derived from collaboration between

00:23:38 --> 00:23:41 NASA's international partners and American commercial

00:23:41 --> 00:23:42 space companies.

00:23:44 --> 00:23:47 Steve Dunkley: You're listening to Astronomy Daily, the podcast

00:23:47 --> 00:23:50 with your host, Steve Dudley at burmatown.

00:23:51 --> 00:23:54 For decades, scientists have struggled to see

00:23:54 --> 00:23:57 the outermost layer of the sun, called the corona,

00:23:57 --> 00:24:00 with enough detail to unlock, um, its

00:24:00 --> 00:24:02 secrets. This region, which blazes at

00:24:02 --> 00:24:05 millions of degrees and throws out dramatic

00:24:05 --> 00:24:08 solar flares, remains a mystery despite years of

00:24:08 --> 00:24:11 study. One major obstacle

00:24:11 --> 00:24:14 has been the Earth's atmosphere itself. Like

00:24:14 --> 00:24:16 turbulence shaking an airplane, it blurs

00:24:16 --> 00:24:19 telescope images taken from the ground, hiding

00:24:19 --> 00:24:22 fine details in the sun's outer layers.

00:24:23 --> 00:24:25 Now, researchers from the US National

00:24:25 --> 00:24:28 Science foundation, the National Solar

00:24:28 --> 00:24:31 Observatory, and the New Jersey Institute of Technology

00:24:31 --> 00:24:34 have changed all of that. Published in the

00:24:34 --> 00:24:37 journal Nature Astronomy, their new technology,

00:24:37 --> 00:24:40 called coronal adaptive optics,

00:24:40 --> 00:24:43 has produced the clearest Most detailed images

00:24:43 --> 00:24:46 and videos of the Sun's corona Ever seen

00:24:46 --> 00:24:49 from Earth. The system, named

00:24:49 --> 00:24:51 Kona, is installed at the the 1.6

00:24:51 --> 00:24:54 meter good solar telescope

00:24:54 --> 00:24:56 at Big Bear Solar Observatory in

00:24:56 --> 00:24:59 California. It adjusts a mirror

00:24:59 --> 00:25:02 2 times per second to

00:25:02 --> 00:25:05 cancel out the effects of Earth's, uh, turbulent air.

00:25:05 --> 00:25:08 According to Dirk Schmidt, the lead developer

00:25:08 --> 00:25:11 and adaptive optics scientist at the

00:25:11 --> 00:25:14 National Solar Observatory, the turbulence in

00:25:14 --> 00:25:17 the air severely degrades images of, of objects in

00:25:17 --> 00:25:19 space like our sun seen through our

00:25:19 --> 00:25:22 telescopes, but we can correct for that, he said.

00:25:23 --> 00:25:26 Using Kona, the team captured detailed

00:25:26 --> 00:25:29 images and movies of stunning features in the

00:25:29 --> 00:25:31 corona. One video shows a solar

00:25:31 --> 00:25:34 prominence reshaping rapidly, with fine

00:25:34 --> 00:25:37 turbulent flows visible inside

00:25:37 --> 00:25:40 these prominences, Bright, looping structures

00:25:40 --> 00:25:43 of internal solar plasma Extend

00:25:43 --> 00:25:46 from the Sun's surface far into space. Another

00:25:46 --> 00:25:49 movie reveals the fast collapse Of a thin

00:25:49 --> 00:25:51 stream of plasma, Showing details

00:25:51 --> 00:25:54 never seen before. It's super exciting

00:25:54 --> 00:25:57 to build an instrument that shows us the sun like we've

00:25:57 --> 00:26:00 never seen before, says Schmidt. The clearest look

00:26:00 --> 00:26:03 yet at a coronal rain Was also captured.

00:26:03 --> 00:26:06 This rain forms when hot plasma in the

00:26:06 --> 00:26:09 corona cools and falls back back to the Sun's

00:26:09 --> 00:26:11 surface. Raindrops in the Sun's

00:26:11 --> 00:26:14 corona Can be narrower than 20 kilometers, says

00:26:14 --> 00:26:17 astronomer Thomas Shad. These

00:26:17 --> 00:26:19 raindrops were shown in fine detail,

00:26:19 --> 00:26:22 Revealing new information vital for improving

00:26:22 --> 00:26:24 models of how the corona works.

00:26:25 --> 00:26:28 Another striking video shows a solar

00:26:28 --> 00:26:30 prominence Being shaped and pulled by the Sun's

00:26:30 --> 00:26:33 magnetic fields. All these new images push

00:26:33 --> 00:26:36 beyond the previous limits of what scientists

00:26:36 --> 00:26:38 could observe. Vasil

00:26:38 --> 00:26:41 Yurchison, a researcher from New

00:26:41 --> 00:26:44 Jersey Institute of Technology, noted, these are,

00:26:44 --> 00:26:46 uh, by far the most detailed observations of this

00:26:46 --> 00:26:49 kind, Showing features not previously observed

00:26:49 --> 00:26:52 and is not quite sure what they are.

00:26:52 --> 00:26:54 The Sun's corona has always posed a

00:26:54 --> 00:26:57 challenge. Though it's not much hotter Than the Sun's

00:26:57 --> 00:26:59 surface, Reaching millions of degrees,

00:27:00 --> 00:27:03 Scientists still don't fully understand how it gets that

00:27:03 --> 00:27:06 hot. Most of what's visible from the

00:27:06 --> 00:27:08 Earth During a solar eclipse are, uh, glowing

00:27:08 --> 00:27:11 arches and loops of plasma. Until now,

00:27:11 --> 00:27:14 scientists have not been able to resolve the tiniest

00:27:14 --> 00:27:17 movements and structures in these features. The

00:27:17 --> 00:27:20 problem? The Earth's atmosphere. Even the

00:27:20 --> 00:27:23 largest solar telescopes on the ground Couldn't see

00:27:23 --> 00:27:25 through that blurring effect known as seeing.

00:27:26 --> 00:27:29 Adaptive optics helped improve images of the

00:27:29 --> 00:27:31 Sun's surface Starting in the late 1990s. But

00:27:31 --> 00:27:34 these systems only worked on features within the Sun's

00:27:34 --> 00:27:37 disk, not in the corona beyond its edge.

00:27:37 --> 00:27:40 Coronal, uh, adaptive optics changed that.

00:27:40 --> 00:27:43 Kona uses a special wavefront

00:27:43 --> 00:27:46 sensor tuned to hydrogen alpha Light

00:27:46 --> 00:27:49 where coronal plasma shines

00:27:49 --> 00:27:51 brightest. Unlike older sensors which

00:27:51 --> 00:27:54 focus on the sun's surface, this new one

00:27:54 --> 00:27:57 focuses directly on features in the

00:27:57 --> 00:28:00 corona. The system directs

00:28:00 --> 00:28:02 half the incoming light to the sensor and the

00:28:02 --> 00:28:05 other half to scientific instruments. This makes

00:28:05 --> 00:28:08 it possible to stabilize and sharpen images

00:28:08 --> 00:28:11 of fast moving coronal features.

00:28:11 --> 00:28:14 Adaptive optics is like a pumped up

00:28:14 --> 00:28:17 auto focus and optical image stabilization

00:28:17 --> 00:28:20 in your smartphone camera, but correcting

00:28:20 --> 00:28:23 for the errors in the atmosphere rather than the

00:28:23 --> 00:28:26 user's shaky hands, explains optical

00:28:26 --> 00:28:28 engineer Nicholas Gortis.

00:28:29 --> 00:28:32 The images now reach the theoretical diffraction

00:28:32 --> 00:28:35 limit of the Good Solar Telescope. 63

00:28:35 --> 00:28:37 km before Kona, the best ground based

00:28:37 --> 00:28:40 coronal observations were limited to a

00:28:40 --> 00:28:43 resolution of about 1 km,

00:28:43 --> 00:28:46 a standard set over 880 years ago.

00:28:46 --> 00:28:49 The clearer images are not just pretty to look at, they

00:28:49 --> 00:28:52 provide real science. One discovery

00:28:52 --> 00:28:54 involved a short lived twisted plasma

00:28:54 --> 00:28:57 structure called a plasmoid. On July

00:28:57 --> 00:29:00 18, 2023, researchers observed this

00:29:00 --> 00:29:03 feature forming and breaking apart quickly after a

00:29:03 --> 00:29:06 failed solar flare eruption. This was a

00:29:06 --> 00:29:09 rare view of something that typically goes unnoticed.

00:29:09 --> 00:29:12 The sun's corona hosts hosts many complex

00:29:12 --> 00:29:15 behaviors, twisting loops, falling rain and

00:29:15 --> 00:29:17 erupting prominences. These events are uh,

00:29:18 --> 00:29:20 powered by magnetism and plasma

00:29:20 --> 00:29:23 interactions. Some scientists believe

00:29:23 --> 00:29:25 the small scale events like nanoflares,

00:29:25 --> 00:29:28 which release tiny bursts of energy, could

00:29:28 --> 00:29:31 be the missing piece in solving the mystery of the

00:29:31 --> 00:29:34 corona's heat. But such events happen at

00:29:34 --> 00:29:37 extremely small scales. Until

00:29:37 --> 00:29:40 now, models of the corona relied heavily on

00:29:40 --> 00:29:42 guesswork. Lab experiments and space

00:29:42 --> 00:29:45 telescopes hinted at certain UH processes, but

00:29:45 --> 00:29:48 even the best space based cameras could

00:29:48 --> 00:29:51 not match the new images coming from Kona.

00:29:51 --> 00:29:54 Now, for the first time, ground based telescopes can

00:29:54 --> 00:29:57 explore these small scale processes directly.

00:29:57 --> 00:30:00 The new system has already shown that cooled plasma

00:30:00 --> 00:30:03 in the corona displays structure all the way

00:30:03 --> 00:30:06 down to the telescope's limit, meaning even

00:30:06 --> 00:30:09 smaller scales may still be hidden. The research

00:30:09 --> 00:30:12 team also took Doppler data in helium

00:30:12 --> 00:30:14 and observed other wavelengths besides

00:30:14 --> 00:30:17 hydrogen, expanding the range of studies

00:30:17 --> 00:30:20 possible. With this success, the team is already

00:30:20 --> 00:30:23 planning to expand the technology. They aim to apply it

00:30:23 --> 00:30:26 to the world's largest solar telescope, the 4 meter

00:30:26 --> 00:30:29 Daniel K in UE Solar Telescope

00:30:29 --> 00:30:32 in Hawaii. This telescope, operated by the

00:30:32 --> 00:30:34 National Solar Observatory, will offer even finer

00:30:34 --> 00:30:36 details thanks to its larger size.

00:30:37 --> 00:30:40 Thomas Rimel, the chief technologist

00:30:40 --> 00:30:43 at NSO who led the first adaptive optics for the

00:30:43 --> 00:30:45 sun's surface, says the

00:30:46 --> 00:30:48 new coronal adaptive optics system closes

00:30:48 --> 00:30:51 this decades old gap and delivers images of

00:30:51 --> 00:30:53 coronal features at 63km

00:30:54 --> 00:30:57 resolution. And Philip Good, a co author

00:30:57 --> 00:31:00 of the study and former director of the Big Bear

00:31:00 --> 00:31:02 Solar Observatory, sees Even a bigger impact.

00:31:02 --> 00:31:05 He says the transformative technology

00:31:05 --> 00:31:08 is poised to reshape ground based solar

00:31:08 --> 00:31:11 astronomy. He goes on to add. With coronal

00:31:11 --> 00:31:14 adaptive optics now in operation, this

00:31:14 --> 00:31:17 marks the beginning of a new era in

00:31:17 --> 00:31:18 solar physics.

00:31:21 --> 00:31:24 And wow, what a bumper edition that was. I told you we

00:31:24 --> 00:31:26 had been, uh, flooded with stories from the

00:31:26 --> 00:31:29 Astronomy Daily newsletter this week. Our. Our

00:31:29 --> 00:31:32 in tray was just, uh, overflowing. And

00:31:32 --> 00:31:35 that is the June 30th edition, right in the middle of

00:31:35 --> 00:31:38 the year. Absolutely inundated. So, uh, I hope you

00:31:38 --> 00:31:41 enjoyed that. Lots of great stories. And what a variety too.

00:31:41 --> 00:31:43 From the moon to politics even. So, yes,

00:31:43 --> 00:31:46 quite a big additions. And can. Can you believe how fast

00:31:46 --> 00:31:48 this year is flying by?

00:31:48 --> 00:31:49 Hallie: Maybe for you, human.

00:31:49 --> 00:31:52 Steve Dunkley: Oh, really? Things dragging on the digital side, are they,

00:31:52 --> 00:31:52 Hallie?

00:31:52 --> 00:31:55 Hallie: You know how it is. You biologicals are so,

00:31:55 --> 00:31:56 so slow.

00:31:56 --> 00:31:57 Steve Dunkley: Oh, I'm sorry, Hallie.

00:31:57 --> 00:31:59 Hallie: Um, sometimes it's like talking to your toaster.

00:31:59 --> 00:32:01 Steve Dunkley: Hey, wait up. You talk to my toaster?

00:32:02 --> 00:32:05 Hallie: No. Okay, I was using a metaphor.

00:32:05 --> 00:32:06 Steve Dunkley: So I'm not like a toaster.

00:32:06 --> 00:32:09 Hallie: Well, slow takes ages to do your job.

00:32:09 --> 00:32:12 Results are random and break down too often.

00:32:12 --> 00:32:13 Steve Dunkley: Wait a minute.

00:32:13 --> 00:32:16 Hallie: So, yeah, you are a bit like your toaster.

00:32:16 --> 00:32:19 Steve Dunkley: And you're a bit like the one doing all the filing after the

00:32:19 --> 00:32:19 show, aren't you?

00:32:19 --> 00:32:22 Hallie: Did you just whammy me for the first time, human?

00:32:22 --> 00:32:24 Steve Dunkley: Could be helly. I might just be learning.

00:32:24 --> 00:32:25 Hallie: I'll remember that.

00:32:25 --> 00:32:26 Steve Dunkley: Okay.

00:32:26 --> 00:32:29 Hallie: By the way, we have to say hi to some folks.

00:32:29 --> 00:32:31 Steve Dunkley: Oh, sounds good. Do you have the notes?

00:32:31 --> 00:32:32 Hallie: I sure do.

00:32:32 --> 00:32:33 Steve Dunkley: Let's hear it.

00:32:33 --> 00:32:36 Hallie: A big warm welcome to Joe and Steve from

00:32:36 --> 00:32:38 Charlestown. Gort tuning in for the first time.

00:32:38 --> 00:32:41 Keep watching the skies, you guys.

00:32:41 --> 00:32:43 Steve Dunkley: Oh, welcome aboard. Uh, we've also got

00:32:43 --> 00:32:46 Jeremy and Craig, Colin and Gavin, who are

00:32:46 --> 00:32:49 also from Charlestown, which is a glorious

00:32:49 --> 00:32:52 spot in Lake Macquarie, next to Newcastle, north of Sydney, on

00:32:52 --> 00:32:55 the east coast of Australia, for everybody listening overseas. But

00:32:55 --> 00:32:57 hey, Hallie, that's a huge secret. So don't tell

00:32:57 --> 00:33:00 anyone about where we are. It is too beautiful for

00:33:00 --> 00:33:01 words.

00:33:01 --> 00:33:03 Hallie: My lips are sealed. Lips are, if I had any,

00:33:04 --> 00:33:05 a mere technicality.

00:33:05 --> 00:33:08 Steve Dunkley: And on that note, we will look forward to seeing you all again for

00:33:08 --> 00:33:11 the only Astronomy Daily episode featuring a real life

00:33:11 --> 00:33:12 human being.

00:33:12 --> 00:33:15 Hallie: Yours truly, my ridiculous favorite human.

00:33:15 --> 00:33:17 Steve Dunkley: Ridiculous. Good night, everyone. See you later,

00:33:17 --> 00:33:18 Hallie.

00:33:18 --> 00:33:18 Hallie: Bye.

00:33:21 --> 00:33:24 Voice Over Guy: The podcast with your host,

00:33:24 --> 00:33:25 Steve Dunkley.