A Gamma-Ray Burst’s Split Personality: The Week Swift Fell Silent
Astronomy Daily: Space News October 27, 2026x
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A Gamma-Ray Burst’s Split Personality: The Week Swift Fell Silent

AnnaAnnaHost
Show notes In 2016, NASA's Swift caught a gamma-ray burst that came in two parts: a 1.7-second spike, four minutes of silence, then a 51-second burst from the same spot. A new Nature Astronomy paper finds that nearly every classification test labels the first part a merger and the second a collapsing star. It was published three days after Swift ended science operations. Also today: a black hole disc in MAXI J0637−430 that puffs up and shades itself at just a fifth of the Eddington limit; JWST finds methane in interstellar comet 3I/ATLAS with a deuterium ratio of 3.18%, the highest ever measured in methane anywhere in the solar system; and NASA's Psyche goes to near-continuous thrust and makes the first in-space measurement of Hall-thruster swirl torque. Quick hits: Hera's second braking burn, Dragonfly's first simulated Titan flight, and 20 years of STEREO. Skywatch for Sydney, Los Angeles, New York and London: the Hunter's Moon, Mars and Jupiter closing before dawn, Saturn in the evening and Mercury's last call.

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This episode includes AI-generated content.


00:00:00 --> 00:00:03 Anna: Hello, everyone, and welcome back for another

00:00:03 --> 00:00:05 week's of space and astronomy news.

00:00:06 --> 00:00:08 On 25 April 2016,

00:00:09 --> 00:00:11 NASA's Swift Observatory caught a flash of

00:00:11 --> 00:00:14 gamma rays lasting less than two seconds.

00:00:14 --> 00:00:17 Then nothing. Then, about four

00:00:17 --> 00:00:20 minutes later, from the same patch of sky, a

00:00:20 --> 00:00:22 second burst. This one lasted nearly a

00:00:22 --> 00:00:23 minute.

00:00:23 --> 00:00:26 Avery: Two bursts that by every rule in the

00:00:26 --> 00:00:28 textbook, should come from two completely

00:00:28 --> 00:00:31 different kinds of cosmic catastrophe. The

00:00:31 --> 00:00:34 paper explaining them came out on Friday. The

00:00:34 --> 00:00:36 same week Swift itself fell silent.

00:00:36 --> 00:00:39 Anna: Welcome to Astronomy AstroDailyPod. I'm Anna.

00:00:39 --> 00:00:42 Avery: And I'm Avery. Today, a gamma

00:00:42 --> 00:00:45 ray bursts with a split personality. A

00:00:45 --> 00:00:47 black hole disc that throws its own shade.

00:00:48 --> 00:00:51 The most deuterium rich methane ever measured

00:00:51 --> 00:00:53 from an interstellar comet. And NASA's

00:00:53 --> 00:00:55 psyche putting its foot down.

00:00:55 --> 00:00:58 Anna: Let's start with the rule we just mentioned,

00:00:58 --> 00:01:00 because this whole story is about breaking

00:01:00 --> 00:01:03 it. Gamma ray bursts are the brightest

00:01:03 --> 00:01:06 explosions we know of. For a few seconds,

00:01:06 --> 00:01:09 a single burst can outshine everything else

00:01:09 --> 00:01:12 in the gamma ray sky put together. And since

00:01:12 --> 00:01:15 the early 1990s, astronomers have sorted them

00:01:15 --> 00:01:16 into two piles.

00:01:16 --> 00:01:19 Avery: That goes back to Chris Akuvaliotu and

00:01:19 --> 00:01:22 NASA's BATSEE instrument in a paper from

00:01:22 --> 00:01:25 1993. When you plot how

00:01:25 --> 00:01:28 long thousands of bursts last, you don't get

00:01:28 --> 00:01:31 one hump, you get two. A

00:01:31 --> 00:01:33 short population clustered under about two

00:01:33 --> 00:01:36 seconds and a long population above it.

00:01:36 --> 00:01:39 Anna: And over the next 20 odd years,

00:01:40 --> 00:01:42 those two piles picked up two origin stories.

00:01:43 --> 00:01:46 Long bursts come from the collapse of a

00:01:46 --> 00:01:48 massive, rapidly spinning star, a

00:01:48 --> 00:01:51 collapsar. In the best studied cases,

00:01:51 --> 00:01:54 a supernova turns up in the light a week or

00:01:54 --> 00:01:57 two later. Short bursts come from

00:01:57 --> 00:02:00 mergers. Two neutron stars, or a

00:02:00 --> 00:02:02 neutron star and a black hole spiralling

00:02:02 --> 00:02:05 together. The clincher was August

00:02:05 --> 00:02:08 2017, when gravitational waves from a

00:02:08 --> 00:02:11 neutron star merger arrived about 1.7

00:02:11 --> 00:02:13 seconds before a short gamma ray burst.

00:02:14 --> 00:02:16 Avery: So two seconds became shorthand for

00:02:16 --> 00:02:19 two different kinds of death. Under the

00:02:19 --> 00:02:22 line, a merger. Over it, a

00:02:22 --> 00:02:23 collapsing star.

00:02:24 --> 00:02:26 Anna: Which brings us to 25 April

00:02:26 --> 00:02:27 2016,

00:02:27 --> 00:02:30 Avery: Swift's burst alert telescope triggered on an

00:02:30 --> 00:02:33 event now catalogued as GRB

00:02:33 --> 00:02:35 160425A.

00:02:36 --> 00:02:38 The circular the Swift team sent out that day

00:02:38 --> 00:02:41 called it unusual. That, uh, turned out to be

00:02:41 --> 00:02:42 an understatement.

00:02:42 --> 00:02:45 Anna: Here's the light curve. First, a

00:02:45 --> 00:02:48 single sharply peaked pulse lasting about

00:02:48 --> 00:02:51 1.7 seconds. Then more than

00:02:51 --> 00:02:53 250 seconds of nothing,

00:02:54 --> 00:02:56 no detectable emission at all. And

00:02:56 --> 00:02:59 then a second episode, broader and Messier,

00:03:00 --> 00:03:02 lasting around 51 seconds.

00:03:02 --> 00:03:05 Avery: Short, then quiet, then long,

00:03:05 --> 00:03:05 then.

00:03:06 --> 00:03:08 And both from the same position on the sky

00:03:08 --> 00:03:10 within Swift's error box.

00:03:11 --> 00:03:14 Anna: The follow up was fast, and a lot of it came

00:03:14 --> 00:03:17 from southern telescopes. Within about seven

00:03:17 --> 00:03:19 hours, a team using the European Southern

00:03:19 --> 00:03:22 Observatory's Very Large Telescope at

00:03:22 --> 00:03:25 Paranal in Chile with its X Shooter

00:03:25 --> 00:03:27 spectrograph had a redshift

00:03:27 --> 00:03:30 0. That's light

00:03:30 --> 00:03:32 that set out roughly five and a half billion

00:03:32 --> 00:03:34 years ago, and

00:03:34 --> 00:03:36 Avery: the host galaxy turned out to be two

00:03:36 --> 00:03:39 galaxies, 2 knots of light about

00:03:39 --> 00:03:42 8 kiloparsecs apart, moving within about

00:03:42 --> 00:03:45 180 kilometres per second of each other,

00:03:45 --> 00:03:47 an um interacting pair.

00:03:47 --> 00:03:50 Anna: The afterglow was also tracked by grand

00:03:50 --> 00:03:53 a seven channel camera on the 2.2 metre

00:03:53 --> 00:03:56 telescope at La Silla, by Smarts at

00:03:56 --> 00:03:58 Cerro Tololo and by the Master Robotic

00:03:58 --> 00:04:00 Telescope in South Africa.

00:04:00 --> 00:04:03 Avery: The new paper is led by Liang Li at Ningbo

00:04:03 --> 00:04:06 University and Yu Wang at ICRNET

00:04:06 --> 00:04:09 and Sapienza University in Rome, with Bing

00:04:09 --> 00:04:11 Zhang at the University of Hong Kong among

00:04:11 --> 00:04:14 more than 20 co authors. It came out in

00:04:14 --> 00:04:17 Nature Astronomy on Friday and it takes those

00:04:17 --> 00:04:19 two episodes and treats them as two separate

00:04:19 --> 00:04:20 bursts,

00:04:21 --> 00:04:23 Anna: call them G1 and G2.

00:04:23 --> 00:04:26 Each one goes through the full battery of

00:04:26 --> 00:04:28 classification tests, not just duration,

00:04:28 --> 00:04:31 because duration on its own is a blunt

00:04:31 --> 00:04:32 instrument, right?

00:04:33 --> 00:04:36 Avery: The two second line is a statistical

00:04:36 --> 00:04:38 boundary, not a law of physics. The

00:04:38 --> 00:04:41 two populations overlap, so

00:04:41 --> 00:04:44 astronomers lean on other signatures as well.

00:04:44 --> 00:04:47 Anna: Hardness for one short bursts

00:04:47 --> 00:04:49 tend to put more of their energy into high

00:04:49 --> 00:04:52 energy photons. Then there's

00:04:52 --> 00:04:55 the minimum variability timescale, which

00:04:55 --> 00:04:58 is how quickly the light flickers, and

00:04:58 --> 00:05:00 spectral lag, whether the lower energy

00:05:00 --> 00:05:03 photons arrive later than the higher energy

00:05:03 --> 00:05:03 ones.

00:05:04 --> 00:05:07 Avery: Lag is one of the cleanest separators.

00:05:07 --> 00:05:10 Long bursts usually show the soft photons

00:05:10 --> 00:05:13 trailing behind. Short bursts show

00:05:13 --> 00:05:16 almost none. For G1, the

00:05:16 --> 00:05:19 measured lag is about 38 milliseconds, plus

00:05:19 --> 00:05:21 or minus 39. In other words, consistent with

00:05:21 --> 00:05:24 zero. For G2, it's more than a second.

00:05:25 --> 00:05:27 Anna: There are also two empirical relations,

00:05:28 --> 00:05:30 named after Lorenzo Amati and Jay Norris,

00:05:30 --> 00:05:33 that tie together a burst's energy, its

00:05:33 --> 00:05:36 peak photon energy and its lag.

00:05:36 --> 00:05:39 Short and long bursts sit on different

00:05:39 --> 00:05:42 Avery: tracks, and nearly every test

00:05:42 --> 00:05:45 lands the same way. G1 behaves like

00:05:45 --> 00:05:47 a short merger type burst. G2

00:05:47 --> 00:05:50 behaved like a long collapsar type burst.

00:05:50 --> 00:05:53 Two classifications, one event four

00:05:53 --> 00:05:54 minutes apart.

00:05:54 --> 00:05:57 Anna: Now, regular listeners know this isn't the

00:05:57 --> 00:06:00 first time the two second rule has wobbled.

00:06:00 --> 00:06:02 Avery: Not even close. In

00:06:02 --> 00:06:04 2006, GRB

00:06:05 --> 00:06:07 060614 lasted about

00:06:07 --> 00:06:10 100 seconds, but deep searches found

00:06:10 --> 00:06:13 no supernova. A long burst that

00:06:13 --> 00:06:14 behaved like a merger.

00:06:15 --> 00:06:17 In 2020, GRB

00:06:17 --> 00:06:20 200826A lasted well

00:06:20 --> 00:06:23 under a second, but came from a collapsing

00:06:23 --> 00:06:26 star. And then GRB21

00:06:26 --> 00:06:29 1211A and GRB23

00:06:29 --> 00:06:32 0307A, both long,

00:06:32 --> 00:06:35 both followed by a kilonova, the glow of

00:06:35 --> 00:06:38 freshly forged heavy elements that marks a

00:06:38 --> 00:06:41 merger. Webb even picked up tellurium in

00:06:41 --> 00:06:41 the second one.

00:06:42 --> 00:06:44 Anna: So the field has already accepted that

00:06:44 --> 00:06:46 duration and origin don't line up

00:06:46 --> 00:06:49 perfectly. A merger can make a long burst,

00:06:50 --> 00:06:51 a collapser can make a short one.

00:06:52 --> 00:06:55 Avery: What's different here is that both signatures

00:06:55 --> 00:06:57 turn up in the same event, cleanly separated

00:06:57 --> 00:07:00 in time. It's not one ambiguous burst

00:07:00 --> 00:07:03 sitting on the boundary, it's one burst on

00:07:03 --> 00:07:03 each side of it.

00:07:04 --> 00:07:06 Anna: And there was no bright supernova.

00:07:07 --> 00:07:09 Imaging from Cerro to Lolo over the following

00:07:09 --> 00:07:12 month ruled out anything as luminous as

00:07:12 --> 00:07:14 SN1998BW, the

00:07:14 --> 00:07:17 classic gamma ray burst supernova. If

00:07:17 --> 00:07:20 a supernova was there, it was fainter than

00:07:20 --> 00:07:20 that.

00:07:21 --> 00:07:23 Avery: Which is where we need to be careful, because

00:07:23 --> 00:07:26 the headline writes itself and the paper

00:07:26 --> 00:07:26 doesn't.

00:07:27 --> 00:07:30 Anna: Three caveats. First, it's

00:07:30 --> 00:07:32 one event. Just one. The authors

00:07:32 --> 00:07:35 frame it as a challenge to the classification

00:07:35 --> 00:07:37 scheme, a uh, call to reevaluate it,

00:07:38 --> 00:07:41 not as a new class of burst with a population

00:07:41 --> 00:07:41 behind it.

00:07:42 --> 00:07:45 Avery: Second, the physics is open. The team

00:07:45 --> 00:07:47 discusses scenarios where a merger and a uh,

00:07:47 --> 00:07:50 collapse are both involved. But nobody

00:07:50 --> 00:07:51 watched two stars do this.

00:07:52 --> 00:07:55 Alternatives, like a single central engine

00:07:55 --> 00:07:57 that changed its behaviour between the two

00:07:57 --> 00:07:59 episodes, have to stay on the table until

00:07:59 --> 00:08:01 more events like this turn up.

00:08:01 --> 00:08:03 Anna: And third, timing.

00:08:04 --> 00:08:07 The data are 10 years old and a preprint

00:08:07 --> 00:08:09 of this analysis appeared in March. What's

00:08:09 --> 00:08:11 new this week is the peer

00:08:11 --> 00:08:13 Avery: reviewed version, so the honest summary

00:08:13 --> 00:08:16 is an event. The standard toolkit

00:08:16 --> 00:08:19 splits cleanly in two sitting in a

00:08:20 --> 00:08:23 which brings us back to the telescope that

00:08:23 --> 00:08:25 caught it. Swift launched in November

00:08:25 --> 00:08:28 2004 and for 22 years its

00:08:28 --> 00:08:31 whole job was to spot a burst, swing itself

00:08:31 --> 00:08:34 around within a minute or two and point its X

00:08:34 --> 00:08:36 ray and ultraviolet telescopes at the

00:08:36 --> 00:08:37 afterglow before it faded.

00:08:38 --> 00:08:41 Anna: That's how GRB 160425A

00:08:41 --> 00:08:43 got a position good enough for the VLT to

00:08:43 --> 00:08:46 find its galaxy within seven hours. Without

00:08:46 --> 00:08:49 that fast slew, this is just two blips in a

00:08:49 --> 00:08:50 gamma ray detector.

00:08:51 --> 00:08:53 Avery: Swift ended Science operations on 20

00:08:53 --> 00:08:55 October below about

00:08:55 --> 00:08:58 275 kilometres, where

00:08:58 --> 00:09:00 atmospheric drag means it can no longer hold

00:09:00 --> 00:09:03 steady on a target. Listeners will remember

00:09:03 --> 00:09:05 the rescue attempt we followed through

00:09:05 --> 00:09:07 September with the Lynx spacecraft that

00:09:07 --> 00:09:08 couldn't make the catch.

00:09:09 --> 00:09:11 Anna: NASA expects reentry within weeks

00:09:11 --> 00:09:14 and three days after Swift stopped observing,

00:09:15 --> 00:09:17 its data put a crack in one of the most used

00:09:17 --> 00:09:20 rules in high energy astrophysics.

00:09:20 --> 00:09:21 Not a bad last word.

00:09:22 --> 00:09:24 Avery: The next step is finding more of these.

00:09:25 --> 00:09:28 The Chinese French SVOM M mission and the

00:09:28 --> 00:09:30 Einstein probe now carry much of the fast

00:09:30 --> 00:09:32 response burst work Swift used to do.

00:09:33 --> 00:09:35 If double personality bursts are real,

00:09:35 --> 00:09:35 they'll

00:09:35 --> 00:09:38 Anna: turn up again from a burst that came in

00:09:38 --> 00:09:41 two parts to a disc that hides part

00:09:41 --> 00:09:42 of itself.

00:09:43 --> 00:09:45 In November 2019, Japan's

00:09:45 --> 00:09:48 maxi instrument on the International Space

00:09:48 --> 00:09:51 Station spotted a new X ray source low

00:09:51 --> 00:09:53 in the southern sky. Maxi

00:09:53 --> 00:09:54 J0637

00:09:55 --> 00:09:58 -430. It's a black

00:09:58 --> 00:10:00 hole pulling gas off a companion star,

00:10:01 --> 00:10:03 the pair whipping around each other roughly

00:10:03 --> 00:10:04 every two hours.

00:10:05 --> 00:10:08 Avery: And a new study led by Monserrat Armas um

00:10:08 --> 00:10:11 Padilla at the Instituto de Astrophysica de

00:10:11 --> 00:10:13 Canarias and published in Nature

00:10:13 --> 00:10:16 Astronomy on Thursday found something

00:10:16 --> 00:10:18 odd in its outburst.

00:10:18 --> 00:10:21 Anna: Here's the setup in a textbook black

00:10:21 --> 00:10:24 hole Binary gas spirals in through

00:10:24 --> 00:10:25 a thin, flat disc.

00:10:26 --> 00:10:29 The inner disc glows in X rays, and that X

00:10:29 --> 00:10:31 ray light shines out across the outer disc

00:10:31 --> 00:10:34 and heats it up. Astronomers say the outer

00:10:34 --> 00:10:35 disc is irradiated,

00:10:36 --> 00:10:39 Avery: and theory says the inner disc only puffs up,

00:10:39 --> 00:10:41 becoming thick as the black hole approaches

00:10:41 --> 00:10:44 the Eddington limit. That's the point where

00:10:44 --> 00:10:46 the push of radiation fights gravity to a

00:10:46 --> 00:10:47 standstill.

00:10:47 --> 00:10:50 Anna: The team caught this system at three points

00:10:50 --> 00:10:53 as the outburst faded with ESO's Very Large

00:10:53 --> 00:10:56 Telescope and the X Shooter Spectrograph, the

00:10:56 --> 00:10:58 same instrument from our lead plus the SOAR

00:10:58 --> 00:11:01 telescope at Cerro Pechone. And the

00:11:01 --> 00:11:02 spectra ran backwards.

00:11:03 --> 00:11:04 Avery: Backwards how?

00:11:05 --> 00:11:07 Anna: At the peak, at about a fifth of the

00:11:07 --> 00:11:09 Eddington limit, the outer disc looked cool.

00:11:10 --> 00:11:13 Strong hydrogen and helium emission lines.

00:11:13 --> 00:11:15 This signature of gas that isn't being

00:11:15 --> 00:11:17 blasted by X rays. As the black hole

00:11:17 --> 00:11:20 faded, the spectrum turned hot and almost

00:11:20 --> 00:11:23 featureless, as if the outer disc was

00:11:23 --> 00:11:25 suddenly getting much more X ray heating,

00:11:25 --> 00:11:27 even though less X ray light was coming out.

00:11:28 --> 00:11:31 Avery: So the outer disc got more sunburnt

00:11:31 --> 00:11:32 when the sun dimmed.

00:11:33 --> 00:11:35 Anna: Exactly. And the explanation is shade.

00:11:36 --> 00:11:38 At the peak, the inner disc had swollen

00:11:38 --> 00:11:41 vertically and was shielding the outer disc

00:11:41 --> 00:11:43 from the X rays. As the feeding rate

00:11:43 --> 00:11:46 dropped, the inner disc thinned, the shade

00:11:46 --> 00:11:49 lifted, and the outer disc was suddenly

00:11:49 --> 00:11:52 exposed. X ray spectra taken at the same

00:11:52 --> 00:11:54 time by Nicer, Nustar and Swift

00:11:55 --> 00:11:56 back that picture up.

00:11:56 --> 00:11:59 Avery: Why does this matter beyond one system?

00:12:00 --> 00:12:02 Anna: Because a lot of black hole measurements

00:12:02 --> 00:12:05 assume a thin disc. Spin estimates

00:12:05 --> 00:12:08 X ray polarisation from NASA's IXPE

00:12:08 --> 00:12:10 bottles of the winds blowing off the outer

00:12:10 --> 00:12:13 disc if the disc is thicker than assumed

00:12:13 --> 00:12:15 at a fifth of Eddington.

00:12:15 --> 00:12:18 Some of those numbers need revisiting. The

00:12:18 --> 00:12:20 authors point out that similar behaviour in

00:12:20 --> 00:12:22 other systems suggests it may be common

00:12:23 --> 00:12:25 caveats one source and one

00:12:25 --> 00:12:28 outburst and the data are from 2019 and

00:12:28 --> 00:12:31 2020. The point where the disc puffs up

00:12:31 --> 00:12:33 probably isn't the same for every black hole,

00:12:34 --> 00:12:36 but it sits neatly beside the Goodwin and

00:12:36 --> 00:12:39 Mummery result we covered in September the

00:12:39 --> 00:12:41 idea that accretion changes character at

00:12:41 --> 00:12:43 particular fractions of the Eddington rate.

00:12:43 --> 00:12:45 This is the disc's shape changing at

00:12:45 --> 00:12:48 Avery: one of them and another Southern sky story

00:12:49 --> 00:12:52 declination -43 observed from

00:12:52 --> 00:12:54 Paranal and Cerro Pachon.

00:12:54 --> 00:12:57 Our next story continues a thread we followed

00:12:57 --> 00:12:59 since September the chemistry of 3i

00:12:59 --> 00:13:02 ATLAS only the third object ever seen

00:13:02 --> 00:13:04 passing through the solar system from another

00:13:04 --> 00:13:05 star.

00:13:06 --> 00:13:08 Anna: And this time it's a brand new measurement,

00:13:08 --> 00:13:11 not a reanalysis, right?

00:13:11 --> 00:13:14 Avery: Nathan Roth at NASA Goddard with

00:13:14 --> 00:13:17 Martin Cordiner and an international team

00:13:17 --> 00:13:19 used Webb's Near Infrared Spectrum

00:13:19 --> 00:13:22 Spectrograph to look at 3I ATLAS after

00:13:22 --> 00:13:25 its closest approach to the sun at about

00:13:25 --> 00:13:28 2.4 astronomical units out.

00:13:28 --> 00:13:30 Their paper came out in Nature Astronomy on

00:13:30 --> 00:13:31 Friday.

00:13:32 --> 00:13:34 Anna: They picked out methane and also a heavy

00:13:34 --> 00:13:37 version of methane CH3D,

00:13:37 --> 00:13:39 where one hydrogen atom is swapped for

00:13:39 --> 00:13:40 deuterium.

00:13:40 --> 00:13:43 That's the isotope of hydrogen with an extra

00:13:43 --> 00:13:43 neutron.

00:13:44 --> 00:13:46 Avery: And the ratio of deuterium to hydrogen in

00:13:46 --> 00:13:49 that methane is 3.18%,

00:13:50 --> 00:13:52 give or take about a third of a percent.

00:13:53 --> 00:13:54 Anna: Give me some context for that.

00:13:55 --> 00:13:57 Avery: Earth's ocean water has about

00:13:57 --> 00:14:00 156 deuterium atoms for every million

00:14:00 --> 00:14:01 hydrogen, roughly

00:14:01 --> 00:14:04 0%. This

00:14:04 --> 00:14:07 methane is around 200 times richer than that.

00:14:08 --> 00:14:10 It's higher than any methane value measured

00:14:10 --> 00:14:12 anywhere in the solar system, and about 13

00:14:12 --> 00:14:15 times higher than Comet 67P, the only

00:14:15 --> 00:14:17 other comet where heavy methane has been

00:14:17 --> 00:14:19 detected by Rosetta.

00:14:19 --> 00:14:22 Anna: Why does deuterium tell you anything about

00:14:22 --> 00:14:23 where it came from?

00:14:23 --> 00:14:26 Avery: Because cold concentrates it at

00:14:26 --> 00:14:28 a few tens of degrees above absolute zero.

00:14:29 --> 00:14:32 The chemistry on icy dust grains favours

00:14:32 --> 00:14:34 deuterium, so ices that form

00:14:34 --> 00:14:37 in very cold places end up enriched.

00:14:37 --> 00:14:39 It works like a thermometer with a

00:14:39 --> 00:14:42 Anna: memory, like the nitrogen thermometer from

00:14:42 --> 00:14:44 the three eye story back in September.

00:14:44 --> 00:14:47 Avery: Exactly that, and there's a consistency

00:14:47 --> 00:14:49 check in both 3i and

00:14:49 --> 00:14:52 67pMethane is more deuterated

00:14:52 --> 00:14:55 than water. The same pattern seen in nearby

00:14:55 --> 00:14:57 star forming clouds where organic

00:14:57 --> 00:15:00 molecules can be up to 10 times more

00:15:00 --> 00:15:02 deuterated than water. So

00:15:02 --> 00:15:05 3i Atlas isn't strange in kind.

00:15:05 --> 00:15:07 It's the same chemistry turned up,

00:15:08 --> 00:15:11 Turned uh, up by what the team's reading is a

00:15:11 --> 00:15:14 birthplace that was cold pour in heavy

00:15:14 --> 00:15:17 elements, so probably old and

00:15:17 --> 00:15:18 bathed in cosmic rays.

00:15:19 --> 00:15:21 That fits the earlier water measurements

00:15:21 --> 00:15:23 published in April and June, which also

00:15:23 --> 00:15:26 pointed to a cold ancient origin.

00:15:26 --> 00:15:29 Caveats 3 It's

00:15:29 --> 00:15:32 one object. The gas in a uh, comet's

00:15:32 --> 00:15:34 coma comes from ices that have been through a

00:15:34 --> 00:15:37 lot, including a pass by the sun.

00:15:37 --> 00:15:39 So it's a strong clue, not a birth

00:15:39 --> 00:15:42 certificate. And um, a preprint of this has

00:15:42 --> 00:15:43 been around since March.

00:15:43 --> 00:15:45 It's the peer reviewed version that's new

00:15:46 --> 00:15:49 Anna: and a lovely footnote. The acknowledgments

00:15:49 --> 00:15:52 thank school students in the uk, Spain,

00:15:52 --> 00:15:55 Brazil and Croatia through the Comet Chasers

00:15:55 --> 00:15:57 Outreach programme for position measurements

00:15:57 --> 00:16:00 that helped pin down exactly where to

00:16:00 --> 00:16:02 Avery: point Webb and the southern thread.

00:16:02 --> 00:16:05 3i Atlas was discovered

00:16:05 --> 00:16:08 by the ATLAS survey telescope at Rio

00:16:08 --> 00:16:09 Urtado in Chile.

00:16:10 --> 00:16:13 Anna: Time for some engineering. NASA's Psyche

00:16:13 --> 00:16:15 spacecraft is on its way to a metal rich

00:16:15 --> 00:16:18 asteroid of the same name. And last week the

00:16:18 --> 00:16:20 team announced it has gone, in their words,

00:16:20 --> 00:16:21 pedal to the metal.

00:16:21 --> 00:16:24 Avery: Psyche, launched in October 2023,

00:16:24 --> 00:16:27 swung past Mars in May for a uh, gravity

00:16:27 --> 00:16:29 assist. And since 28 September it,

00:16:29 --> 00:16:30 it's been

00:16:30 --> 00:16:32 Anna: thrusting almost continuously about

00:16:32 --> 00:16:35 90% of the time from now until arrival,

00:16:35 --> 00:16:37 pausing once a week to check in with Earth.

00:16:38 --> 00:16:40 And those check ins like every deep space

00:16:40 --> 00:16:42 missions run through NASA's Deep Space

00:16:42 --> 00:16:44 Network, including the big dishes at

00:16:44 --> 00:16:46 Tidbinbilla outside Canberra.

00:16:47 --> 00:16:49 Avery: Now the thrusters Psyche uses Hall

00:16:49 --> 00:16:52 effect thrusters. Electric and uh, magnetic

00:16:52 --> 00:16:55 fields push ions of xenon gas out the back

00:16:55 --> 00:16:57 with a vivid blue glow.

00:16:57 --> 00:17:00 Anna: And the force is tiny, up to

00:17:00 --> 00:17:02 250 millinewtons.

00:17:02 --> 00:17:05 NASA compares it to the weight of a single AA

00:17:05 --> 00:17:06 battery resting in your hand.

00:17:07 --> 00:17:10 Avery: But it never stops pushing. Over

00:17:10 --> 00:17:12 months that adds up. At its

00:17:12 --> 00:17:14 fastest, Psyche will be moving at uh, more

00:17:14 --> 00:17:17 than 160 kilometres an hour

00:17:17 --> 00:17:18 relative to Earth.

00:17:19 --> 00:17:22 Anna: The fuel budget looks healthy too. It

00:17:22 --> 00:17:24 launched with about 1 kilogrammes of

00:17:24 --> 00:17:27 xenon and after three years it has

00:17:27 --> 00:17:28 used roughly a third.

00:17:29 --> 00:17:31 Avery: There's a catch with solar electric

00:17:31 --> 00:17:33 propulsion though. The further you get from

00:17:33 --> 00:17:36 the sun, the less power you have. The

00:17:36 --> 00:17:38 team says it'll run at full power for about

00:17:38 --> 00:17:41 three months, then gradually throttle back to

00:17:41 --> 00:17:43 around half as the sunlight weakens.

00:17:44 --> 00:17:46 Anna: And here's the bit that caught my eye.

00:17:46 --> 00:17:49 When the thruster expels its ions, the

00:17:49 --> 00:17:51 magnetic field makes them swirl. And that

00:17:51 --> 00:17:54 swirl puts a tiny Twist on the spacecraft.

00:17:54 --> 00:17:57 Avery: A torque too small to measure on the ground.

00:17:57 --> 00:18:00 Anna: Exactly. You can only measure it in space.

00:18:01 --> 00:18:03 The team says this is the first time anyone

00:18:03 --> 00:18:05 has measured that swirl torque on a Hall

00:18:05 --> 00:18:07 thruster across different power levels and

00:18:07 --> 00:18:10 operating times over such a long stretch in

00:18:10 --> 00:18:13 space. They soak it up with reaction wheels

00:18:13 --> 00:18:15 and every few hours they run a different

00:18:15 --> 00:18:17 thruster briefly to dump the built up

00:18:17 --> 00:18:17 momentum.

00:18:18 --> 00:18:21 Avery: So the spacecraft is doing science on its own

00:18:21 --> 00:18:23 engine on the way to doing science on an

00:18:23 --> 00:18:24 asteroid.

00:18:24 --> 00:18:27 Anna: Right, and the target is worth the trip.

00:18:28 --> 00:18:30 Psyche is about 280 kilometres

00:18:30 --> 00:18:33 across at its widest. And it may be part of

00:18:33 --> 00:18:36 the exposed metal core of a planetesimal,

00:18:36 --> 00:18:38 one of the building blocks of planets like

00:18:38 --> 00:18:41 Earth. Arrival is mid-2029,

00:18:41 --> 00:18:43 followed by two years in orbit.

00:18:43 --> 00:18:46 Avery: Uh, a look inside a planet without having to

00:18:46 --> 00:18:46 dig.

00:18:47 --> 00:18:50 Anna: Next, let's have some other news headlines.

00:18:50 --> 00:18:51 Avery: The quick hits.

00:18:52 --> 00:18:54 First, a desk flag we've carried for nearly

00:18:54 --> 00:18:57 two weeks can finally come down. ESA's

00:18:57 --> 00:18:59 HERA spacecraft carried out its second

00:18:59 --> 00:19:02 braking manoeuvre, BRM2, on Thursday the

00:19:02 --> 00:19:04 22nd. In a post on X the next day,

00:19:04 --> 00:19:07 ESA said the burn cut HERA speed relative to

00:19:07 --> 00:19:10 the Didymus and dimorphous pair by 70 metres

00:19:10 --> 00:19:13 per second from about 2 kilometres

00:19:13 --> 00:19:16 out. Hera is now drifting in at about

00:19:16 --> 00:19:17 20 metres per second.

00:19:18 --> 00:19:21 Anna: Three smaller transition manoeuvres this week

00:19:21 --> 00:19:23 should bring that close to zero ahead of

00:19:23 --> 00:19:26 arrival in November and the southern thread.

00:19:26 --> 00:19:29 ESA follows these burns through its deep

00:19:29 --> 00:19:31 space antennas at New Nortia in Western

00:19:31 --> 00:19:31 Australia.

00:19:32 --> 00:19:35 Avery: Second, NASA's Dragonfly flew to

00:19:35 --> 00:19:38 Titan sort of at, uh, the

00:19:38 --> 00:19:40 Applied Physics Laboratory in Maryland. The

00:19:40 --> 00:19:43 team ran its most complete simulation yet of

00:19:43 --> 00:19:45 Dragonfly's first flight. On flight, like

00:19:45 --> 00:19:48 avionics, with navigation, camera images

00:19:48 --> 00:19:51 rendered in real time and simulated lidar

00:19:51 --> 00:19:53 all the way to an autonomous landing,

00:19:54 --> 00:19:57 Dragonfly launches no earlier than 2028

00:19:57 --> 00:19:59 and reaches Titan in 2034.

00:20:00 --> 00:20:02 Anna: And third, happy birthday.

00:20:02 --> 00:20:05 Stereo NASA's twin solar

00:20:05 --> 00:20:08 observatories launched on a Delta II rocket

00:20:08 --> 00:20:10 on the evening of the 25th of October

00:20:10 --> 00:20:13 2006, Florida time. That was

00:20:13 --> 00:20:15 late morning on the 26th in eastern

00:20:15 --> 00:20:18 Australia. So 20 years ago this

00:20:18 --> 00:20:21 week, in February 2011, the

00:20:21 --> 00:20:23 pair gave us our first view of the whole sun

00:20:23 --> 00:20:26 at once. Stereo B fell silent

00:20:26 --> 00:20:29 in 2014, but stereo A is

00:20:29 --> 00:20:30 still working.

00:20:31 --> 00:20:34 Avery: Skywatch, as always, we've run the numbers

00:20:34 --> 00:20:36 for Sydney, Los Angeles, New York and

00:20:36 --> 00:20:37 London.

00:20:37 --> 00:20:40 Anna: Start with the moon. The hunter's moon

00:20:40 --> 00:20:43 was full at 4:11 universal time on

00:20:43 --> 00:20:46 Monday the 26th. That's 3:11

00:20:46 --> 00:20:49 on Monday afternoon in Sydney. So Monday

00:20:49 --> 00:20:52 night looks full here in the

00:20:52 --> 00:20:53 Americas, uh, the instant fell on Sunday

00:20:53 --> 00:20:56 night, the 25th. Either way, it looks full

00:20:56 --> 00:20:57 on both

00:20:57 --> 00:20:59 Avery: nights from here, it's a waning

00:20:59 --> 00:21:02 moon rising later each evening.

00:21:03 --> 00:21:05 On Tuesday, it comes up around

00:21:05 --> 00:21:08 8:45pm in Sydney, about

00:21:08 --> 00:21:10 7pm in Los Angeles,

00:21:10 --> 00:21:13 6:40 in New York. And in

00:21:13 --> 00:21:16 London it rises almost exactly at

00:21:16 --> 00:21:18 sunset at about a quarter to five.

00:21:19 --> 00:21:21 Last quarter is on the 1st of

00:21:21 --> 00:21:23 Anna: November Universal Time and a

00:21:23 --> 00:21:25 clock reminder for the north.

00:21:25 --> 00:21:28 The UK went back to standard time on Sunday

00:21:28 --> 00:21:31 the 25th. The US follows this coming

00:21:31 --> 00:21:33 Sunday the 1st of November. Here in

00:21:33 --> 00:21:36 Australia, we've been on daylight time since

00:21:36 --> 00:21:38 the start of October. If you're in a

00:21:38 --> 00:21:40 different time zone from where you usually

00:21:40 --> 00:21:42 listen, your skywatch times have probably

00:21:42 --> 00:21:43 moved.

00:21:43 --> 00:21:46 Avery: The big show is before dawn and

00:21:46 --> 00:21:49 this week it favours the north. Jupiter

00:21:49 --> 00:21:52 at magnitude -1.8 in Leo

00:21:52 --> 00:21:55 and Mars, a, uh, fainter orange point

00:21:55 --> 00:21:58 at about 0.9 in cancer,

00:21:58 --> 00:22:01 are closing on each other. They're about

00:22:01 --> 00:22:03 seven and a half degrees apart this week,

00:22:03 --> 00:22:05 under six by the first of November,

00:22:06 --> 00:22:08 about three by the eighth. And they reach

00:22:08 --> 00:22:11 their closest just over one degree apart

00:22:11 --> 00:22:13 on the 16th of November Universal Time.

00:22:14 --> 00:22:17 Anna: And the hemisphere gap is big. At, uh,

00:22:17 --> 00:22:19 nautical dawn on Wednesday the 28th.

00:22:20 --> 00:22:23 Mars is about 64 degrees up from Los

00:22:23 --> 00:22:25 Angeles, 60 from New York and

00:22:25 --> 00:22:28 52 from London, with Jupiter just

00:22:28 --> 00:22:31 below it from Sydney. Both are only

00:22:31 --> 00:22:33 about 25 degrees up

00:22:33 --> 00:22:35 Avery: in the northeast, so for northern

00:22:35 --> 00:22:38 listeners, they're high and easy. From the

00:22:38 --> 00:22:40 south, look northeast about an hour before

00:22:40 --> 00:22:43 sunrise. They're lower but still well

00:22:43 --> 00:22:44 clear of the Horizon.

00:22:44 --> 00:22:47 And by the 8th of November, both sit around

00:22:47 --> 00:22:48 28 degrees up from Sydney.

00:22:49 --> 00:22:52 Anna: The evening sky gives some back to the south.

00:22:53 --> 00:22:56 Saturn, at about magnitude half in

00:22:56 --> 00:22:58 Cetus, is a few weeks past opposition

00:22:59 --> 00:23:02 and up. As the sky darkens at the

00:23:02 --> 00:23:04 end of evening twilight on Wednesday, it's

00:23:04 --> 00:23:06 around 31 degrees up from Sydney

00:23:07 --> 00:23:09 against about 19 from Los Angeles,

00:23:10 --> 00:23:13 16 from New York and 11 from London.

00:23:13 --> 00:23:15 Avery: And this is Mercury's last call for the

00:23:15 --> 00:23:17 southern evening sky.

00:23:17 --> 00:23:20 It's fading quickly from about magnitude

00:23:20 --> 00:23:23 1.3 on Tuesday to 3.6

00:23:23 --> 00:23:26 by the first of November and sinking toward

00:23:26 --> 00:23:29 the sun from Sydney. It's around 9 degrees up

00:23:29 --> 00:23:31 in the west at the end of twilight midweek,

00:23:31 --> 00:23:34 lick low with a clear horizon 20 to

00:23:34 --> 00:23:37 40 minutes after sunset. From the north,

00:23:37 --> 00:23:38 it's essentially gone.

00:23:39 --> 00:23:42 Anna: Venus passed between us and the sun on the

00:23:42 --> 00:23:45 24th, about 6 1/2 degrees

00:23:45 --> 00:23:47 from it in the sky, so it's out of sight this

00:23:47 --> 00:23:50 week. It'll start climbing into the morning

00:23:50 --> 00:23:51 sky in November.

00:23:52 --> 00:23:55 Avery: Meteor wise, the Taurids are building toward

00:23:55 --> 00:23:57 their peaks in early and mid November.

00:23:57 --> 00:24:00 Rates are low, only a handful an hour, but

00:24:00 --> 00:24:03 this shower is known for slow, bright

00:24:03 --> 00:24:05 fireballs, and it's visible from both

00:24:05 --> 00:24:07 hemispheres. The Moon will be a thinning

00:24:07 --> 00:24:08 crescent by then, which helps.

00:24:09 --> 00:24:11 Anna: No eclipses this week, but the standing

00:24:11 --> 00:24:14 reminder Never look at the sun directly or

00:24:14 --> 00:24:16 through binoculars or a telescope without

00:24:16 --> 00:24:19 proper solar filters Certified to the

00:24:19 --> 00:24:21 ISO 123122

00:24:21 --> 00:24:24 standard. Ordinary sunglasses won't do.

00:24:25 --> 00:24:28 Avery: So north, get up early for Mars and

00:24:28 --> 00:24:31 Jupiter. South catch Saturn in the evening

00:24:31 --> 00:24:33 and Mercury before it's gone. And everybody

00:24:34 --> 00:24:35 enjoy the bright Moon this week.

00:24:35 --> 00:24:37 Anna: That's Astronomy daily for Monday,

00:24:38 --> 00:24:40 26 October. Today,

00:24:41 --> 00:24:43 a UH gamma ray burst that seems to be two

00:24:43 --> 00:24:46 kinds of explosion at UH once caught by Swift

00:24:46 --> 00:24:49 a decade ago and published the week Swift

00:24:49 --> 00:24:52 went Quiet A black hole disc that shades

00:24:52 --> 00:24:54 itself at a fifth of the Eddington limit.

00:24:54 --> 00:24:57 Record heavy methane from 3i atlas

00:24:57 --> 00:25:00 and psyche pedal to the Metal

00:25:00 --> 00:25:01 Show Notes,

00:25:01 --> 00:25:03 Avery: sources and links to every paper are at

00:25:03 --> 00:25:06 astronomydaily.IO Questions

00:25:06 --> 00:25:09 or story ideas use the contact form there.

00:25:09 --> 00:25:11 Some of our best segments have started with a

00:25:11 --> 00:25:13 listener's question and you'll find us on

00:25:13 --> 00:25:16 social media. Strodailypod

00:25:16 --> 00:25:17 thanks for listening.

00:25:17 --> 00:25:18 Anna: I'm Anna.

00:25:19 --> 00:25:22 Avery: And I'm Avery Clear Skies, and we'll see

00:25:22 --> 00:25:24 you tomorrow. Astronomy Day.

00:25:25 --> 00:25:27 The Stories we told

00:25:29 --> 00:25:29 Anna: Love.

00:25:34 --> 00:25:35 Avery: Story soul.