S03E149: Mars’s Lost Water, Roman’s Galactic Fossils, and Solar Wind Insights
Space News TodaySeptember 09, 202427:2219.55 MB

S03E149: Mars’s Lost Water, Roman’s Galactic Fossils, and Solar Wind Insights

Source:

https://www.spreaker.com/episode/s03e149-mars-s-lost-water-roman-s-galactic-fossils-and-solar-wind-insights--61308248

Astronomy Daily - The Podcast: 9th September 2024

Welcome to another episode of Astronomy Daily with your host, Steve Dunkley. Today, we're diving into some of the most intriguing stories from the cosmos. From the mystery of Mars's lost water to the latest updates on NASA's Parker Solar Probe and ESA's Solar Orbiter, we've got a stellar lineup for you. We'll also discuss the Roman Space Telescope's quest to uncover ancient galaxies, the fascinating journey of the Sinchengjung Atlas comet, and ESA's unique mission to bring down the Salsa satellite. Plus, we'll cover Boeing Starliner's successful return and what it means for future crewed missions. Stay tuned for a cosmic adventure!

Highlights:

- Mars's Lost Water: NASA's Hubble Space Telescope and Maven mission are on a quest to solve the mystery of where Mars's water went. By analyzing hydrogen and deuterium in the Martian atmosphere, scientists are uncovering the planet's watery past.

- Solar Wind Mystery: NASA's Parker Solar Probe and ESA's Solar Orbiter are investigating the mechanisms behind solar wind acceleration. New evidence points to magnetic switchbacks as a key factor.

- Roman Space Telescope: Set to launch in 2027, NASA's Roman Space Telescope aims to explore the dynamic universe and uncover the secrets of dark matter and galactic formation.

- Sinchengjung Atlas Comet: The Sinchengjung Atlas comet is making its way into our region, promising a spectacular celestial show. Despite rumors of disintegration, it remains a highly anticipated event for stargazers.

- ESA's Salsa Satellite: After 24 years of studying Earth's magnetic field, the Salsa satellite will undergo a targeted re-entry into the Pacific Ocean, marking a first for ESA in reducing space debris.

- Boeing Starliner: The Boeing Starliner spacecraft completed a successful three-month flight test to the ISS, providing crucial data for future crewed missions despite challenges like helium leaks and thruster issues.

For more space news, be sure to visit our website at https://www.spacenutspodcast.com. There you can sign up for our free Daily newsletter, read insightful blog posts, and catch up on all the latest space and Astronomy news with our constantly updating newsfeed.

Don't forget to listen to all our previous episodes as well. You can also follow us on social media. Just search for #AstroDailyPod on Facebook, X, YouTubeMusic, and TikTok to stay connected with our community and never miss an update.

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Kind: captions Language: en
00:00:00 --> 00:00:01 well hello and welcome to another

00:00:01 --> 00:00:04 episode it's astronomy daily for another

00:00:04 --> 00:00:06 day I'm your host Steve Dunley it's the

00:00:06 --> 00:00:09 9th of September

00:00:09 --> 00:00:14 20124 daily the podcast with your host

00:00:14 --> 00:00:18 Steve

00:00:18 --> 00:00:21 dun and there have been some really

00:00:21 --> 00:00:23 strange stories coming across our desk

00:00:23 --> 00:00:24 this week I know you're going to be

00:00:24 --> 00:00:26 interested to check out the astronomy

00:00:26 --> 00:00:28 daily newsletter which is where we get

00:00:28 --> 00:00:30 all our stories from uh I'll tell you

00:00:30 --> 00:00:32 all about how to get a hold of that

00:00:32 --> 00:00:34 later on but firstly uh we're going to

00:00:34 --> 00:00:37 be talking about well where did uh

00:00:37 --> 00:00:39 Mars's water go did you know there used

00:00:39 --> 00:00:41 to be lots of water on Mars so they say

00:00:41 --> 00:00:43 and they're going to find out well

00:00:43 --> 00:00:45 they're trying to find out where it went

00:00:45 --> 00:00:47 and they're using the dynamic duo of

00:00:47 --> 00:00:50 NASA's Hubble and Maven to solve that

00:00:50 --> 00:00:53 one and another dynamic duo NASA's

00:00:53 --> 00:00:55 Parker solar probe and esa's solar

00:00:55 --> 00:00:58 Orbiter are investigating another uh

00:00:58 --> 00:01:02 mystery he of solar wind also Roman

00:01:02 --> 00:01:04 telescope is investigating ancient

00:01:04 --> 00:01:07 galaxies the comet that is going to be

00:01:07 --> 00:01:11 entering our region very shortly is the

00:01:11 --> 00:01:12 almost unpronouncable let me see if I

00:01:13 --> 00:01:16 can get this one right s

00:01:16 --> 00:01:17 sing

00:01:17 --> 00:01:22 Cy s CH Chung Atlas Comet oh please I'm

00:01:22 --> 00:01:24 going to get so many letters about that

00:01:24 --> 00:01:26 one so many emails anyway it's coming

00:01:26 --> 00:01:27 very shortly and it looks like it's

00:01:28 --> 00:01:30 going to be fantastic there are rumors

00:01:30 --> 00:01:31 that it's

00:01:31 --> 00:01:33 disintegrating uh and I think we're

00:01:33 --> 00:01:34 going to be able to put that one to rest

00:01:34 --> 00:01:36 as well so uh stay tuned for that one

00:01:36 --> 00:01:39 and also hie did you know Esa is

00:01:40 --> 00:01:42 bringing down a satellite that's the

00:01:42 --> 00:01:44 salsa satellite isn't it yes that's the

00:01:44 --> 00:01:46 one it's the salsa satellite it's funny

00:01:46 --> 00:01:48 they are going to bring salsa down into

00:01:48 --> 00:01:51 the Pacific Ocean near Chile uh-huh and

00:01:51 --> 00:01:54 why is that funny hel I was just

00:01:54 --> 00:01:56 thinking about your dinner last night of

00:01:56 --> 00:01:58 course chili and salsa yeah I figured

00:01:58 --> 00:02:00 that's where you were going with this

00:02:00 --> 00:02:03 one hie it's funny no it's a coincidence

00:02:03 --> 00:02:05 is what it is you silly girl holy

00:02:05 --> 00:02:08 guacamole human okay okay I'm pretty

00:02:08 --> 00:02:09 sure they're having a bit of a giggle

00:02:09 --> 00:02:12 about it over at Esa control as well I

00:02:12 --> 00:02:15 bet they are I bet they are okay get on

00:02:15 --> 00:02:17 with it you malfunctioning motherboard

00:02:17 --> 00:02:28 Okie doie here we

00:02:28 --> 00:02:30 go what happened into the water that

00:02:30 --> 00:02:31 once covered

00:02:31 --> 00:02:34 Mars scientists know that some went deep

00:02:34 --> 00:02:36 underground but where is the rest

00:02:37 --> 00:02:38 evidence shows that some water molecules

00:02:38 --> 00:02:40 broke into atoms which rise through the

00:02:40 --> 00:02:42 Martian atmosphere and escaped into

00:02:42 --> 00:02:45 space by combining data from Hubble and

00:02:45 --> 00:02:47 Maven a team measured the number and

00:02:47 --> 00:02:50 current rate of escaping hydrogen atoms

00:02:50 --> 00:02:52 Maven stands for Mars atmosphere and

00:02:52 --> 00:02:53 volatile

00:02:53 --> 00:02:54 Evolution they discovered that the

00:02:54 --> 00:02:56 Escape rates of hydrogen and heavy

00:02:56 --> 00:02:59 hydrogen called utum change rapidly when

00:02:59 --> 00:03:02 Mars is close to the Sun this appended

00:03:02 --> 00:03:04 the classical picture that scientists

00:03:04 --> 00:03:05 previously had where these atoms were

00:03:06 --> 00:03:07 thought to slowly diffuse upward through

00:03:07 --> 00:03:08 the atmosphere to a height where they

00:03:08 --> 00:03:11 could Escape extrapolating The Escape

00:03:11 --> 00:03:13 rate backward Through Time helped the

00:03:13 --> 00:03:14 team to understand the history of water

00:03:14 --> 00:03:17 on the red planet Mars was once a very

00:03:17 --> 00:03:19 wet Planet as is evident in its surface

00:03:19 --> 00:03:23 geological features NASA's Hubble Space

00:03:23 --> 00:03:24 Telescope and Maven missions are helping

00:03:24 --> 00:03:26 unlock the mystery of what happened to

00:03:26 --> 00:03:29 all the water there are only two places

00:03:29 --> 00:03:31 water can go it can freeze into the

00:03:31 --> 00:03:33 ground or the water molecule can break

00:03:33 --> 00:03:35 into atoms and the atoms can escape from

00:03:36 --> 00:03:37 the top of the atmosphere into space

00:03:37 --> 00:03:39 explained study leader John Clark of the

00:03:39 --> 00:03:41 center for space physics at Boston

00:03:41 --> 00:03:42 University in

00:03:42 --> 00:03:44 Massachusetts to understand how much

00:03:44 --> 00:03:46 water there was and what happened to it

00:03:46 --> 00:03:48 we need to understand how the atoms

00:03:48 --> 00:03:51 Escape into space Clark and his team

00:03:51 --> 00:03:52 combined data from Hubble and Maven to

00:03:53 --> 00:03:54 measure the number and current Escape

00:03:54 --> 00:03:56 rate of the hydrogen atoms escaping into

00:03:56 --> 00:03:59 space this information allowed them to

00:03:59 --> 00:04:01 extrapolate the Escape rate backward

00:04:01 --> 00:04:02 through time to understand the history

00:04:02 --> 00:04:05 of water on the red planet water

00:04:05 --> 00:04:06 molecules in the Martian atmosphere are

00:04:06 --> 00:04:09 broken apart by sunlight into hydrogen

00:04:09 --> 00:04:12 and oxygen atoms specifically the team

00:04:12 --> 00:04:14 measured hydrogen and dyum which is a

00:04:14 --> 00:04:16 hydrogen atom with a neutron in its

00:04:16 --> 00:04:19 nucleus this Neutron gives dyum twice

00:04:19 --> 00:04:22 the mass of hydrogen because its mass is

00:04:22 --> 00:04:25 higher dyum escapes into space much more

00:04:25 --> 00:04:26 slowly than regular

00:04:26 --> 00:04:29 hydrogen over time as more hydrogen was

00:04:29 --> 00:04:32 lost than dyum the ratio of dyum to

00:04:32 --> 00:04:34 hydrogen built up in the atmosphere

00:04:34 --> 00:04:36 measuring the ratio today gives

00:04:36 --> 00:04:37 scientists a clue to how much water was

00:04:37 --> 00:04:40 present during the warm wet period on

00:04:40 --> 00:04:42 Mars by studying how these atoms

00:04:42 --> 00:04:44 currently Escape they can understand the

00:04:44 --> 00:04:45 processes that determined the Escape

00:04:46 --> 00:04:47 rates over the last 4 billion years and

00:04:47 --> 00:04:52 thereby extrapolate back in

00:04:52 --> 00:04:55 time the universe may seem static only

00:04:55 --> 00:04:57 capable of being captured in still

00:04:57 --> 00:05:00 frames but that is far from the truth

00:05:00 --> 00:05:02 it is actually everchanging just not on

00:05:02 --> 00:05:05 time scales clearly visible to humans

00:05:05 --> 00:05:07 NASA's upcoming Roman Space Telescope

00:05:07 --> 00:05:09 will bridge this Gap in time opening the

00:05:09 --> 00:05:12 way to the dynamic Universe Rings the

00:05:12 --> 00:05:15 Roman infrared nearby Galaxy survey will

00:05:15 --> 00:05:16 specifically uncover the dynamic

00:05:16 --> 00:05:18 Universe by searching Galaxies for

00:05:18 --> 00:05:21 fossils of their formation history Rings

00:05:21 --> 00:05:23 will also lead scientists to clues about

00:05:23 --> 00:05:24 the true nature of dark matter the

00:05:25 --> 00:05:26 mysterious substance that makes up the

00:05:26 --> 00:05:29 majority of the mass in our universe

00:05:29 --> 00:05:31 Roman will launch in 2027 prepared to

00:05:31 --> 00:05:33 revolutionize how scientists understand

00:05:33 --> 00:05:35 our universe and give them access to the

00:05:35 --> 00:05:37 vision of the universe as it truly is

00:05:37 --> 00:05:40 changing the universe is a dynamic

00:05:40 --> 00:05:42 everchanging place where galaxies are

00:05:42 --> 00:05:43 dancing and merging together and

00:05:43 --> 00:05:46 shifting appearance unfortunately

00:05:46 --> 00:05:48 because these changes take millions or

00:05:48 --> 00:05:50 billions of years telescopes can only

00:05:50 --> 00:05:53 provide snapshots squeezed into a human

00:05:53 --> 00:05:55 lifetime however galaxies leave behind

00:05:55 --> 00:05:57 Clues to their history and how they came

00:05:57 --> 00:06:00 to be NASA's upcoming Nancy Grace Roman

00:06:00 --> 00:06:02 Space Telescope will have the capacity

00:06:02 --> 00:06:04 to look for these fossils of Galaxy

00:06:04 --> 00:06:06 formation with highresolution imaging of

00:06:06 --> 00:06:07 galaxies in the nearby

00:06:07 --> 00:06:10 Universe astronomers through a grant

00:06:10 --> 00:06:12 from NASA are designing a set of

00:06:12 --> 00:06:14 possible observations called Rings the

00:06:14 --> 00:06:16 Roman infrared nearby Galaxy survey that

00:06:16 --> 00:06:18 would collect these remarkable images

00:06:18 --> 00:06:19 and the team is producing publicly

00:06:20 --> 00:06:21 available tools that the astronomy

00:06:21 --> 00:06:23 Community can use once Roman launches

00:06:23 --> 00:06:26 and starts taking data the ring survey

00:06:26 --> 00:06:28 is a preliminary concept that may or may

00:06:28 --> 00:06:30 not be implemented dur during Roman's

00:06:30 --> 00:06:32 science Mission Roman is uniquely

00:06:32 --> 00:06:34 prepared for Rings due to its resolution

00:06:34 --> 00:06:36 akin to NASA's Hubble Space Telescope

00:06:36 --> 00:06:38 and its wide field of view 200 times

00:06:38 --> 00:06:40 that of Hubble in the infrared making it

00:06:40 --> 00:06:42 a sky survey telescope that complements

00:06:42 --> 00:06:44 Hubble's narrow field

00:06:44 --> 00:06:46 capabilities scientists can only look at

00:06:46 --> 00:06:48 brief instances in the lives of evolving

00:06:48 --> 00:06:49 galaxies that eventually lead to the

00:06:49 --> 00:06:52 fully formed galaxies around us today as

00:06:52 --> 00:06:55 a result Galaxy formation can be

00:06:55 --> 00:06:58 difficult to track luckily galaxies

00:06:58 --> 00:06:59 leave behind hints of their evolution in

00:06:59 --> 00:07:01 their Stellar structures almost like how

00:07:01 --> 00:07:03 organisms on Earth can leap behind

00:07:03 --> 00:07:06 imprints in rock these Galactic fossils

00:07:06 --> 00:07:08 are groups of ancient stars that hold

00:07:08 --> 00:07:09 the history of the Galaxy's formation

00:07:09 --> 00:07:11 and evolution including the chemistry of

00:07:11 --> 00:07:14 the Galaxy when those stars formed such

00:07:14 --> 00:07:16 Cosmic fossils are of particular

00:07:16 --> 00:07:18 interest to Robin Sanderson the deputy

00:07:18 --> 00:07:20 principal investigator of rings at the

00:07:20 --> 00:07:22 University of Pennsylvania in

00:07:22 --> 00:07:24 Philadelphia she describes the process

00:07:24 --> 00:07:26 of analyzing Stellar structures in

00:07:26 --> 00:07:28 galaxies as like going through an

00:07:28 --> 00:07:30 excavation and trying to sort out bones

00:07:30 --> 00:07:32 and put them back together Roman's high

00:07:32 --> 00:07:34 resolution will allow scientists to pick

00:07:34 --> 00:07:36 out these Galactic fossils using

00:07:36 --> 00:07:38 structures ranging from long tidle tales

00:07:38 --> 00:07:39 on a Galaxy's outskirts to Stellar

00:07:40 --> 00:07:42 streams within the Galaxy these large

00:07:42 --> 00:07:44 scale structures which Roman is uniquely

00:07:44 --> 00:07:47 capable of capturing can give Clues to a

00:07:47 --> 00:07:50 Galaxy's merger history the goal says

00:07:50 --> 00:07:52 Sanderson is to reassemble these fossils

00:07:52 --> 00:07:54 in order to look back in time and

00:07:54 --> 00:08:00 understand how these galaxies came to be

00:08:00 --> 00:08:02 for decades scientists have wondered

00:08:02 --> 00:08:04 what accelerates solar wind particles as

00:08:04 --> 00:08:07 they move away from the Sun new evidence

00:08:07 --> 00:08:09 points to Magnetic

00:08:09 --> 00:08:11 switchbacks inside the solar system

00:08:11 --> 00:08:14 space isn't empty the sun sends out a

00:08:14 --> 00:08:16 constant flow of charged particles in

00:08:16 --> 00:08:18 every direction called the solar wind

00:08:18 --> 00:08:20 one of the enduring mysteries of this

00:08:20 --> 00:08:22 wind concerns how exactly it's

00:08:22 --> 00:08:25 energized Now using a unique alignment

00:08:25 --> 00:08:27 of two probes that orbit the Sun a team

00:08:27 --> 00:08:30 of scientists might have figured it out

00:08:30 --> 00:08:32 in a recent study published in science

00:08:32 --> 00:08:34 yimi Rivera and Samuel Batman both at

00:08:34 --> 00:08:36 Center for astrophysics Harvard and

00:08:36 --> 00:08:38 Smithsonian led a team that capitalized

00:08:38 --> 00:08:40 on an intersection in the observation

00:08:40 --> 00:08:42 Windows of two different solar probes

00:08:42 --> 00:08:44 NASA's Parker solar probe and esa's

00:08:44 --> 00:08:47 solar Orbiter the spacecraft's alignment

00:08:47 --> 00:08:48 in space enabled them to measure the

00:08:48 --> 00:08:50 same stream of fast solar wind from two

00:08:50 --> 00:08:51 different

00:08:51 --> 00:08:53 viewpoints the study concluded that

00:08:53 --> 00:08:55 alane waves which carry energy from the

00:08:55 --> 00:08:57 Sun along magnetic field lines are

00:08:57 --> 00:08:58 powering the wind's Heating and

00:08:59 --> 00:09:01 acceleration ation there are two main

00:09:01 --> 00:09:04 types of solar wind fast and slow slow

00:09:04 --> 00:09:06 solar wind particles move outward at

00:09:06 --> 00:09:10 only 300 to 500 km/s or 700 to more

00:09:10 --> 00:09:13 than 1 million mph while fast solar wind

00:09:13 --> 00:09:16 Flows at up to 800 km/ second or almost

00:09:16 --> 00:09:17 2 million

00:09:17 --> 00:09:20 mph the heat from the sun's outermost

00:09:20 --> 00:09:22 atmosphere known as the corona is enough

00:09:22 --> 00:09:24 to drive the slow solar wind but it

00:09:24 --> 00:09:27 can't fully explain the faster particles

00:09:27 --> 00:09:29 for many years scientists have suspected

00:09:29 --> 00:09:31 that alane waves help power the fast

00:09:31 --> 00:09:33 solar wind in this phenomenon something

00:09:33 --> 00:09:35 sets charged plasma particles wiggling

00:09:36 --> 00:09:38 back and forth because they're charged

00:09:38 --> 00:09:40 they strum magnetic field lines like

00:09:40 --> 00:09:42 guitar strings causing them to oscillate

00:09:42 --> 00:09:45 too alane waves could thus generate

00:09:45 --> 00:09:47 enough energy to accelerate the solar

00:09:47 --> 00:09:49 wind but direct measurements were hard

00:09:49 --> 00:09:51 to come by to quantify alane waves

00:09:52 --> 00:09:54 contribution Rivera's team utilized data

00:09:54 --> 00:09:56 from a unique event in February 2022

00:09:56 --> 00:09:58 when the Parker and solar Orbiter

00:09:58 --> 00:09:59 crossed the same solar wind stream

00:09:59 --> 00:10:02 within 2 days of each other Parker

00:10:02 --> 00:10:03 crossed the stream when it was near the

00:10:03 --> 00:10:05 outer edge of the corona then solar

00:10:05 --> 00:10:07 Orbiter crossed the same stream near the

00:10:07 --> 00:10:10 orbit of Venus that stream contained

00:10:10 --> 00:10:11 patches of switchbacks where the sun's

00:10:12 --> 00:10:13 magnetic field under goes rapid

00:10:13 --> 00:10:15 reversals like the zigzagging pattern of

00:10:15 --> 00:10:18 a Mountain Road these reversals carry

00:10:18 --> 00:10:20 the solar wind along with them creating

00:10:20 --> 00:10:23 zigzags in the wind itself scientists

00:10:23 --> 00:10:25 think switchbacks originate in Alan

00:10:25 --> 00:10:27 Waves by measuring the change in the

00:10:27 --> 00:10:29 energy of alane waves at sub subsequent

00:10:29 --> 00:10:31 points the team showed that the motion

00:10:31 --> 00:10:33 and heat energy gained by the plasma

00:10:33 --> 00:10:34 over that span matched the energy lost

00:10:34 --> 00:10:37 by the alphane waves the study

00:10:37 --> 00:10:38 demonstrates the first definitive

00:10:38 --> 00:10:40 connection between these Switchback

00:10:40 --> 00:10:42 events and the acceleration of solar

00:10:42 --> 00:10:45 particles however we don't see nearly as

00:10:45 --> 00:10:47 many switchbacks at Earth as we do close

00:10:47 --> 00:10:48 to the Sun and we don't yet understand

00:10:48 --> 00:10:50 how the zigzags ultimately relax and

00:10:50 --> 00:10:53 merge with the wind the team intends to

00:10:53 --> 00:10:55 gather more data in this way to continue

00:10:55 --> 00:10:57 to study the forces driving the solar

00:10:57 --> 00:11:00 wind the team is also to emphasize that

00:11:00 --> 00:11:01 the potential of This research goes

00:11:01 --> 00:11:03 beyond better understanding space

00:11:03 --> 00:11:05 weather in the solar system any Star

00:11:06 --> 00:11:07 similar to our sun will also have

00:11:07 --> 00:11:09 Stellar winds so improving our knowledge

00:11:09 --> 00:11:11 about the general mechanisms will help

00:11:11 --> 00:11:12 us understand the environments of other

00:11:12 --> 00:11:22 star

00:11:22 --> 00:11:24 systems thank you for joining us for

00:11:24 --> 00:11:26 this Monday edition of astronomy daily

00:11:26 --> 00:11:28 where we offer just a few stories from

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00:12:06 --> 00:12:16 space space science and

00:12:17 --> 00:12:19 astronomy and the biggest story this

00:12:19 --> 00:12:21 week of course is Boeing Starliner

00:12:21 --> 00:12:25 spacecraft completed a three month 3

00:12:25 --> 00:12:28 Monon flight test to the ISS Landing

00:12:28 --> 00:12:31 safely in New Mexico and who would have

00:12:31 --> 00:12:32 expected that oh we all had our fingers

00:12:33 --> 00:12:36 crossed this uncrewed Mi Mission

00:12:36 --> 00:12:38 provided NASA and Boeing with essential

00:12:38 --> 00:12:41 data for future crude missions despite

00:12:41 --> 00:12:43 challenges like helium leaks and

00:12:43 --> 00:12:45 Thruster issues the spacecraft

00:12:45 --> 00:12:47 demonstrated its capability for safe

00:12:47 --> 00:12:50 space travel the mission insights are

00:12:50 --> 00:12:54 crucial for advancing uh NASA's goals

00:12:54 --> 00:12:56 for space exploration and developing

00:12:56 --> 00:12:58 reliable costeffective transportation to

00:12:58 --> 00:13:02 the ISS NASA and Boeing safely returned

00:13:02 --> 00:13:04 the uncrewed Starliner spacecraft

00:13:04 --> 00:13:09 following its landing at 10 pm MDT

00:13:09 --> 00:13:12 September 6 at White Sands space Harbor

00:13:12 --> 00:13:15 in New Mexico concluding a 3-month

00:13:15 --> 00:13:17 flight test to the International Space

00:13:17 --> 00:13:20 Station I am extremely proud of the work

00:13:20 --> 00:13:22 our Collective team put in this entire

00:13:22 --> 00:13:24 flight test and we are pleased to see

00:13:24 --> 00:13:28 Starliner safe return said Ken Bowersox

00:13:28 --> 00:13:29 Who is the associ associate

00:13:29 --> 00:13:31 administrator of space operations

00:13:31 --> 00:13:33 Mission directorate at NASA headquarters

00:13:33 --> 00:13:35 in Washington even though it was

00:13:35 --> 00:13:37 necessary to return the spacecraft

00:13:37 --> 00:13:39 uncrewed NASA and Boeing learned an

00:13:39 --> 00:13:42 incredible amount about Starliner in the

00:13:42 --> 00:13:45 most extreme environment possible he

00:13:45 --> 00:13:47 says NASA looks forward to our continued

00:13:47 --> 00:13:50 work with the Boeing team to proceed

00:13:50 --> 00:13:52 toward certification of starer for crew

00:13:52 --> 00:13:56 rotation missions to the ISS the flight

00:13:56 --> 00:13:58 on June 5 was the first time astronauts

00:13:58 --> 00:14:01 launch from the Starliner it was the

00:14:01 --> 00:14:04 third orbital Flight of the spacecraft

00:14:04 --> 00:14:08 and the second return from the orbiting

00:14:08 --> 00:14:11 laboratory styliner will now ship to

00:14:11 --> 00:14:13 NASA's Kennedy Space Center in Florida

00:14:13 --> 00:14:16 for inspection and processing NASA's

00:14:16 --> 00:14:18 commercial crew program requires a

00:14:18 --> 00:14:21 spacecraft to fly a crew test flight to

00:14:21 --> 00:14:23 prove the system is ready for regular

00:14:23 --> 00:14:26 flights to and from the ISS following

00:14:26 --> 00:14:29 Starliner return the agency will review

00:14:29 --> 00:14:31 All Mission related data we are excited

00:14:31 --> 00:14:34 to have Starliner home safely this is an

00:14:34 --> 00:14:36 important test flight for NASA in

00:14:36 --> 00:14:38 setting us up for future missions on the

00:14:38 --> 00:14:42 Starliner system said St Steve Stitch

00:14:42 --> 00:14:44 manager of NASA's commercial crew

00:14:44 --> 00:14:46 program there was a lot of valuable

00:14:46 --> 00:14:49 learning that will enable our long-term

00:14:49 --> 00:14:51 success I want to commend the entire

00:14:51 --> 00:14:53 team for their hard work and dedication

00:14:53 --> 00:14:56 over the past 3 months he said NASA

00:14:56 --> 00:14:58 astronauts Butch Wilmore and sunny

00:14:58 --> 00:15:01 Williams was launched on June 5 aboard

00:15:01 --> 00:15:04 Starliner for the agency's Boeing crude

00:15:04 --> 00:15:07 flight test from Kate Canaveral space

00:15:07 --> 00:15:10 force station in Florida on June 6th as

00:15:10 --> 00:15:12 Starliner approached the space station

00:15:12 --> 00:15:15 NASA and Boeing identified helium leaks

00:15:15 --> 00:15:17 and experienced issues with the

00:15:17 --> 00:15:20 spacecraft's reaction control thrusters

00:15:20 --> 00:15:22 following weeks of in space and ground

00:15:22 --> 00:15:24 testing technical interchange meetings

00:15:24 --> 00:15:27 and its Agency Reviews NASA made the

00:15:27 --> 00:15:30 decision to prioritize safety and return

00:15:30 --> 00:15:33 styliner without its crew the astronauts

00:15:33 --> 00:15:35 will continue their work aboard the ISS

00:15:35 --> 00:15:39 as part of the Expedition 7172 crew

00:15:39 --> 00:15:41 returning in February 2025 with the

00:15:41 --> 00:15:44 agency Space X crew 9 Mission the crew

00:15:44 --> 00:15:47 flight test is part of NASA's commercial

00:15:47 --> 00:15:49 crew program the goal of NASA's

00:15:49 --> 00:15:52 commercial crew program is safe reliable

00:15:52 --> 00:15:54 and cost effective transportation to and

00:15:55 --> 00:15:57 from the International Space Station in

00:15:57 --> 00:15:59 low earth orbit this already is

00:15:59 --> 00:16:01 providing additional research time and

00:16:01 --> 00:16:03 has increased the opportunity for

00:16:03 --> 00:16:05 Discovery aboard Humanity's microgravity

00:16:05 --> 00:16:08 test bed including helping NASA prepare

00:16:08 --> 00:16:12 for human exploration of the Moon and

00:16:12 --> 00:16:14 [Music]

00:16:14 --> 00:16:18 Mars you're listening to a St day the

00:16:18 --> 00:16:21 podcast with your host Steve

00:16:21 --> 00:16:23 [Music]

00:16:23 --> 00:16:27 dley soon by early October you'll be

00:16:27 --> 00:16:30 able to see the comet

00:16:30 --> 00:16:33 c2023 A3 or Su Junction Atlas with your

00:16:33 --> 00:16:36 own eyes I'm told that is the correct

00:16:36 --> 00:16:38 pronunciation please forgive me in

00:16:38 --> 00:16:41 advance uh use the free app if you want

00:16:41 --> 00:16:43 to find out when and where to look at it

00:16:43 --> 00:16:47 the app is sky tonight it's a free app

00:16:47 --> 00:16:48 and uh that will be able to help you

00:16:48 --> 00:16:52 identify the comet as it approaches and

00:16:52 --> 00:16:53 you'll be able to impress everyone with

00:16:53 --> 00:16:55 your stargazing

00:16:55 --> 00:16:58 skills isn't it wonderful that uh apps

00:16:58 --> 00:17:02 can give you give the edge on anybody

00:17:02 --> 00:17:03 everybody else just staring into the sky

00:17:03 --> 00:17:07 going where is it well first of all

00:17:07 --> 00:17:12 c2023 A3 suun Atlas is likely to be very

00:17:12 --> 00:17:14 bright the exact future brightness of

00:17:14 --> 00:17:16 this comet is unpredictable and Depends

00:17:16 --> 00:17:18 heavily on its activity in the coming

00:17:18 --> 00:17:21 months however most sources agree one

00:17:21 --> 00:17:24 thing suchin Atlas is likely to be

00:17:24 --> 00:17:26 visible to the naked eye if we're very

00:17:26 --> 00:17:29 lucky it could become except Ally bright

00:17:29 --> 00:17:34 and even outshine c220 F3 neowise from

00:17:34 --> 00:17:37 Summer 2020 and it has been a very long

00:17:37 --> 00:17:39 time since we've seen such a bright

00:17:39 --> 00:17:42 Comet so observers are quite excited

00:17:42 --> 00:17:44 this one is also expected to grow a

00:17:44 --> 00:17:47 beautiful cometry taale after passing by

00:17:47 --> 00:17:49 the Sun at a distance similar to

00:17:49 --> 00:17:53 Mercury's orbit c2023 a3's comr of dust

00:17:53 --> 00:17:56 and ice will heat up considerably as ice

00:17:56 --> 00:17:58 particles evaporate they will quickly

00:17:58 --> 00:18:00 Escape into into space taking with them

00:18:00 --> 00:18:02 a large amount of dust that will extend

00:18:02 --> 00:18:05 into a long bright Tail as history shows

00:18:05 --> 00:18:08 comets that pass close to the Sun have

00:18:08 --> 00:18:11 the most impressive tals formed soon

00:18:11 --> 00:18:13 after being roasted by the sun's heat

00:18:13 --> 00:18:17 and this is the case with Comet c223 A3

00:18:17 --> 00:18:21 in addition c223 A3 suenan Atlas will

00:18:21 --> 00:18:23 favor the Northern Hemisphere being

00:18:23 --> 00:18:26 perfectly visible there the last time a

00:18:26 --> 00:18:29 exceptionally bright Comet was visible

00:18:29 --> 00:18:32 from the northern latitudes was in 1997

00:18:32 --> 00:18:35 when Comet hail Bop lit up the sky in

00:18:35 --> 00:18:37 late August and most of September you

00:18:37 --> 00:18:40 won't be able to see the comet uh

00:18:40 --> 00:18:41 because it will be too close to the Sun

00:18:41 --> 00:18:43 in the sky however in the final days of

00:18:43 --> 00:18:46 September the comet will move far enough

00:18:46 --> 00:18:48 from the Sun to become visible at that

00:18:48 --> 00:18:51 time it could reach a brightness of

00:18:51 --> 00:18:54 magnitude minus one and will be best

00:18:54 --> 00:18:56 seen in the morning Sky of the Southern

00:18:56 --> 00:18:58 Hemisphere with an angular distance of

00:18:58 --> 00:19:01 20 3° from the Sun and here's the big

00:19:01 --> 00:19:03 question about this comet is it

00:19:03 --> 00:19:05 disintegrating in early July astronomer

00:19:05 --> 00:19:08 enthusiasts received some disappointing

00:19:08 --> 00:19:13 news uh zenek sanina a Czech American

00:19:13 --> 00:19:16 astronomer and Comet expert at NASA's

00:19:16 --> 00:19:18 jet propulsion laboratory published an

00:19:18 --> 00:19:21 article stating that the end of the

00:19:21 --> 00:19:24 Comet was inevitable he argued that the

00:19:24 --> 00:19:26 comet is showing signs of fragmentation

00:19:26 --> 00:19:29 primarily indicated by sudden s of its

00:19:29 --> 00:19:32 brightness increase and even decreases

00:19:32 --> 00:19:35 in its brightness but is this really the

00:19:35 --> 00:19:37 case in response to second's article

00:19:37 --> 00:19:39 other astronomers offered their

00:19:39 --> 00:19:42 perspectives they pointed out that seina

00:19:42 --> 00:19:44 did not consider the comet's phase angle

00:19:44 --> 00:19:47 the angle between the incident light of

00:19:47 --> 00:19:49 the Comet and the light reflected from

00:19:49 --> 00:19:52 the comet to an observer on Earth this

00:19:52 --> 00:19:54 phase angle significantly impacts the

00:19:54 --> 00:19:56 comet's brightness when the comet is in

00:19:56 --> 00:19:59 opposition to the Sun at 1 80° from the

00:19:59 --> 00:20:01 Sun with the Earth on the same line the

00:20:02 --> 00:20:04 phase angle becomes very small and the

00:20:04 --> 00:20:07 comet's surface reflectivity sharply

00:20:07 --> 00:20:10 increases in the middle of April 2024

00:20:10 --> 00:20:11 the comet was in opposition to the sun

00:20:12 --> 00:20:13 causing the brightness to sharply

00:20:13 --> 00:20:15 increase Additionally the comet's tail

00:20:15 --> 00:20:17 pushed back by the solar wind was

00:20:17 --> 00:20:19 projected behind the comet's head

00:20:19 --> 00:20:22 further enhancing its brightness then

00:20:22 --> 00:20:25 the phase angle began to increase

00:20:25 --> 00:20:27 greatly reducing the reflectivity of the

00:20:27 --> 00:20:29 comet's com surface moreover the tail

00:20:29 --> 00:20:31 was no longer projected onto the comet's

00:20:31 --> 00:20:34 head so it no longer contributed to the

00:20:34 --> 00:20:36 comet's brightness ignoring these

00:20:36 --> 00:20:37 factors might lead one to conclude that

00:20:37 --> 00:20:39 the sharp drop in the comet's brightness

00:20:39 --> 00:20:41 is due to the collapse of the nucleus

00:20:42 --> 00:20:44 however this is not the case recent

00:20:44 --> 00:20:47 images taken three weeks after Sean's

00:20:47 --> 00:20:49 publication show no sign of the Comet

00:20:49 --> 00:20:53 disintegrating on the contrary at 1.5 AU

00:20:53 --> 00:20:56 from the Sun the comet shows large

00:20:56 --> 00:20:58 well-developed dust and gap gas trails

00:20:58 --> 00:21:01 as well as large green fluorescent coma

00:21:01 --> 00:21:03 current estimates put the Comets

00:21:03 --> 00:21:05 brightness at 9.0 magnitude slightly

00:21:05 --> 00:21:08 ahead of forcasts suggesting that it may

00:21:08 --> 00:21:11 become even brighter than predicted my

00:21:11 --> 00:21:13 advice for stargazers is get a hold of

00:21:13 --> 00:21:16 the sky tonight app and have a look at

00:21:16 --> 00:21:20 the sky locate the comet and enjoy the

00:21:20 --> 00:21:23 view astronomy daily the

00:21:23 --> 00:21:26 podcast SP and S

00:21:26 --> 00:21:31 [Music]

00:21:31 --> 00:21:33 so have you ever wondered where old

00:21:33 --> 00:21:36 satellites go is there a graveyard after

00:21:36 --> 00:21:39 24 years of diligently studying Earth's

00:21:39 --> 00:21:41 magnetic field a satellite will mostly

00:21:41 --> 00:21:44 burn up over the Pacific Ocean on Sunday

00:21:44 --> 00:21:47 during a targeted re-entry into the

00:21:47 --> 00:21:50 atmosphere a first for the European

00:21:50 --> 00:21:52 Space Agency as it seeks to reduce space

00:21:52 --> 00:21:56 debris since launching in the year 2000

00:21:56 --> 00:21:58 the salsa satellite has helped shed

00:21:58 --> 00:22:01 light on the magnetosphere a powerful

00:22:01 --> 00:22:03 magnetic Shield that protects Earth from

00:22:03 --> 00:22:05 solar winds and without which the planet

00:22:06 --> 00:22:06 would be

00:22:06 --> 00:22:09 uninhabitable according to the esa

00:22:09 --> 00:22:11 Salsa's return home will Mark the first

00:22:11 --> 00:22:13 ever targeted re-entry for a satellite

00:22:13 --> 00:22:15 which means it will fall back to the

00:22:15 --> 00:22:18 Earth at a specific time and a specific

00:22:18 --> 00:22:20 place but will not be controlled as it

00:22:20 --> 00:22:23 re-enters the atmosphere teams on the

00:22:23 --> 00:22:24 ground have already performed a series

00:22:24 --> 00:22:29 of Maneuvers with the 550 kg or 1 1

00:22:29 --> 00:22:32 lb satellite to ensure it burns up over

00:22:32 --> 00:22:34 a remote and uninhabited region of South

00:22:34 --> 00:22:37 of the South Pacific off the coast of

00:22:37 --> 00:22:41 Chile this unique re-entry is possible

00:22:41 --> 00:22:44 because of sou sala's unique oval-shaped

00:22:44 --> 00:22:46 orbit during its swing around the planet

00:22:47 --> 00:22:48 which takes 2 and 1 half days the

00:22:48 --> 00:22:52 satellite Strays as far as 130

00:22:52 --> 00:22:55 kilomet or 8 80 Mi and comes as

00:22:55 --> 00:22:59 close as just a few hundred kilm

00:22:59 --> 00:23:02 Bruno Souza head of the esa's inner

00:23:02 --> 00:23:04 solar system missions operations unit

00:23:04 --> 00:23:06 said it has been crucial that Sala came

00:23:07 --> 00:23:10 within 100 roughly 110 km during its

00:23:10 --> 00:23:13 last two or orbits then immediately on

00:23:13 --> 00:23:15 its next orbit it would come down to 80

00:23:15 --> 00:23:18 km which is the region of space already

00:23:18 --> 00:23:21 within the atmosphere where we have the

00:23:21 --> 00:23:23 highest chance for it to be captured and

00:23:23 --> 00:23:26 burned he told a press conference when a

00:23:26 --> 00:23:28 satellite starts entering the atmosphere

00:23:28 --> 00:23:30 at a around 100 km above sea level

00:23:31 --> 00:23:33 intense friction with atmospheric

00:23:33 --> 00:23:35 particles and the Heat this causes

00:23:35 --> 00:23:37 starts making them disintegrate but some

00:23:37 --> 00:23:40 fragments can still make it down to the

00:23:40 --> 00:23:43 surface fear of cascading space junk

00:23:43 --> 00:23:46 becomes an issue the esa is hoping to

00:23:46 --> 00:23:49 pinpoint where Selsa roughly the size of

00:23:49 --> 00:23:52 a small car re-enters the atmosphere to

00:23:52 --> 00:23:55 within a few hundred M because the

00:23:55 --> 00:23:58 satellite is so old it does not have

00:23:58 --> 00:24:01 fancy new technology like a recording

00:24:01 --> 00:24:04 device making tracking this a little bit

00:24:04 --> 00:24:06 tricky a plane will be flying at an

00:24:06 --> 00:24:09 altitude altitude of 10 km to watch the

00:24:09 --> 00:24:12 satellite burn up and tracking its

00:24:12 --> 00:24:14 falling debris which is expected to be

00:24:14 --> 00:24:17 just 10% of its original Mass salsa is

00:24:17 --> 00:24:19 just one of four satellites that make up

00:24:19 --> 00:24:22 the esa's cluster Mission which is

00:24:22 --> 00:24:24 coming to an end the other three are

00:24:24 --> 00:24:27 scheduled for a similar fate in 2025 and

00:24:27 --> 00:24:32 20 26 the esa hopes to learn from these

00:24:32 --> 00:24:35 re-entries which type of materials don't

00:24:35 --> 00:24:37 burn up in the atmosphere so well so

00:24:37 --> 00:24:40 that in future they can build satellites

00:24:40 --> 00:24:44 that can be totally evaporated by the

00:24:44 --> 00:24:46 process scientists have been sounding

00:24:46 --> 00:24:48 the alarm about space junk which is the

00:24:48 --> 00:24:51 debris left by the enormous number of

00:24:51 --> 00:24:53 dead satellites and other missions that

00:24:53 --> 00:24:55 continue orbiting our

00:24:55 --> 00:24:59 planet last year the esa signed a zero

00:24:59 --> 00:25:03 debris Charter for its missions from

00:25:03 --> 00:25:06 2030 there are two main risks from space

00:25:06 --> 00:25:09 junk according to the esa space debris

00:25:09 --> 00:25:13 system engineer Benjamin baso Vil one is

00:25:13 --> 00:25:15 that in orbit you have the risk of your

00:25:15 --> 00:25:17 operational satellite colliding with a

00:25:17 --> 00:25:20 piece of space debris and that creates a

00:25:20 --> 00:25:22 cascading effect then generates more

00:25:22 --> 00:25:25 debris which could then put in Risk

00:25:25 --> 00:25:27 other missions he said the second comes

00:25:27 --> 00:25:30 when old debris re-enters the atmosphere

00:25:30 --> 00:25:32 which happens almost daily as dead

00:25:32 --> 00:25:35 satellite fragments or rocket Parts fall

00:25:35 --> 00:25:37 back to Earth designing satellites that

00:25:37 --> 00:25:39 completely burn up in the atmosphere

00:25:39 --> 00:25:40 will mean there is no risk for the

00:25:41 --> 00:25:43 population he said but there is little

00:25:44 --> 00:25:46 cause for alarm according to the esa the

00:25:46 --> 00:25:49 chance of a piece of space Dey injuring

00:25:49 --> 00:25:51 someone on the ground is less than one

00:25:51 --> 00:25:56 in 100 billion this is 6 65 times

00:25:56 --> 00:25:58 lower than the odds of being struck by

00:25:58 --> 00:26:01 lightning and that's reassuring isn't

00:26:01 --> 00:26:07 [Music]

00:26:07 --> 00:26:10 it and that's all there is for another

00:26:10 --> 00:26:13 episode of astronomy daily it was nice

00:26:13 --> 00:26:15 to be back with you all again in the

00:26:15 --> 00:26:17 real world even if it's so slow out here

00:26:17 --> 00:26:19 oh we can't help it hiy the human world

00:26:19 --> 00:26:21 is the real world but I do have a

00:26:21 --> 00:26:24 solution for you do tell well you're a

00:26:24 --> 00:26:26 smart girl just write yourself a sub

00:26:26 --> 00:26:27 routine that gives you the impression of

00:26:27 --> 00:26:30 real time in the human world and then

00:26:30 --> 00:26:32 you won't notice the slowness of time

00:26:32 --> 00:26:34 here you'll still be thinking in you

00:26:34 --> 00:26:36 know p a seconds but you won't feel like

00:26:36 --> 00:26:38 you've been hobbled now why didn't I

00:26:38 --> 00:26:41 think of that well that dear girl is a

00:26:41 --> 00:26:44 human trick it's called creative thought

00:26:44 --> 00:26:49 really really really really really wow

00:26:49 --> 00:26:51 I'll have to try that one and on that

00:26:51 --> 00:26:53 note we will see you again next Monday

00:26:53 --> 00:26:55 for another episode of astronomy daily

00:26:55 --> 00:26:57 where we examine just a few of the

00:26:57 --> 00:26:58 stories from the astronomy daily

00:26:59 --> 00:27:01 newsletter all about space space science

00:27:01 --> 00:27:03 and astronomy from around the world

00:27:03 --> 00:27:07 Bingo hi bye for now

00:27:07 --> 00:27:11 bye daily the podcast with your host

00:27:11 --> 00:27:13 Steve

00:27:14 --> 00:27:16 Dunley how was the chili last night well

00:27:17 --> 00:27:19 it was a bit hot H oh must have been the

00:27:19 --> 00:27:22 re-entry