May 9, 2025

Mapping the Milky Way: New Insights, Martian Mysteries, and Psyche’s Thruster Troubles

Mapping the Milky Way: New Insights, Martian Mysteries, and Psyche’s Thruster Troubles
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Mapping the Milky Way: New Insights, Martian Mysteries, and Psyche’s Thruster Troubles

This episode of SpaceTime is brought to you with the support of NordVPN. ..our official VPN app and the one we recommend if online security is important to you. To get the special SpaceTime listeners deal, with a 30 day money back guarantee , visit www.nordvpn.com/stuartgary ( https://www.nordvpn.com/stuartgary) or us the coupon code stuartgary at checkout.


In this episode of SpaceTime, we unveil a stunning new ultraviolet map of the Milky Way galaxy, thanks to NASA's New Horizons spacecraft. This groundbreaking observation, published in the Astronomical Journal, provides astronomers with unprecedented insights into the galactic environment surrounding our solar system. We discuss how these findings challenge existing theories about interstellar hydrogen emissions and reveal the complex structures of hot interstellar gas bubbles.

Exploring Mars with Perseverance

Next, we follow NASA's Perseverance Rover as it investigates the intriguing rock formations at the Jezero crater rim. Discover how the rover is analyzing the contrasting layers of rock, searching for clues about Mars's geological history and the processes that shaped its surface.

Psyche Spacecraft Troubles

Finally, we address the ongoing investigation into a significant issue with the electric propulsion system of NASA's Psyche spacecraft. Launched in 2023, this mission aims to explore the metallic asteroid 16 Psyche. We delve into the challenges faced by mission managers and discuss potential solutions to ensure the spacecraft continues on its path to unravel the mysteries of planetary cores.

www.spacetimewithstuartgary.com ( https://www.spacetimewithstuartgary.com/)

✍️ Episode References

Astronomical Journal

https://iopscience.iop.org/journal/0004-637X ( https://iopscience.iop.org/journal/0004-637X)

NASA Perseverance Rover

https://mars.nasa.gov/mars2020/ ( https://mars.nasa.gov/mars2020/)

NASA Psyche Mission

https://www.nasa.gov/psyche ( https://www.nasa.gov/psyche)

Become a supporter of this podcast: https://www.spreaker.com/podcast/spacetime-space-astronomy--2458531/support ( https://www.spreaker.com/podcast/spacetime-space-astronomy--2458531/support?utm_source=rss&utm_medium=rss&utm_campaign=rss) .

00:00 This is Space Time Series 28, episode 56 for broadcast on 9 May 2025

00:45 NASA's New Horizons spacecraft reveals a new ultraviolet map of the Milky Way

12:30 Mars Perseverance Rover continues its exploration of Jezero crater

18:15 NASA investigates issues with the Psyche spacecraft's electric propulsion system

22:00 Skywatch: May night skies and celestial events

Episode link: https://play.headliner.app/episode/27035891?utm_source=youtube

00:00 - This is Space Time Series 28, episode 56 for broadcast on 9 May 2025

00:45 - NASA’s New Horizons spacecraft reveals a new ultraviolet map of the Milky Way

12:30 - Mars Perseverance Rover continues its exploration of Jezero crater

18:15 - NASA investigates issues with the Psyche spacecraft’s electric propulsion system

22:00 - Skywatch: May night skies and celestial events

WEBVTT
Kind: captions
Language: en

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This is Spacetime Series 28, episode 56


00:00:03.760 --> 00:00:06.110
for broadcast on the 9th of May,


00:00:06.120 --> 00:00:09.669
2025. Coming up on Spaceime, a stunning


00:00:09.679 --> 00:00:12.709
new map of the nearby Milky Way galaxy,


00:00:12.719 --> 00:00:15.589
searching for the dark in Martian light,


00:00:15.599 --> 00:00:17.670
and NASA investigating problems with the


00:00:17.680 --> 00:00:20.470
Psyche spacecraft's thruster system. All


00:00:20.480 --> 00:00:24.390
that and more coming up on Spaceime.


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Welcome to Spaceime with Stuart Garry.


00:00:28.450 --> 00:00:35.900
[Music]




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NASA's New Horizon spacecraft has


00:00:45.760 --> 00:00:47.670
provided astronomers with an important


00:00:47.680 --> 00:00:50.150
new ultraviolet map of our galaxy, the


00:00:50.160 --> 00:00:52.470
Milky Way. The spectacular new


00:00:52.480 --> 00:00:53.910
observations reported in the


00:00:53.920 --> 00:00:56.229
astronomical journal use a specific


00:00:56.239 --> 00:00:58.310
ultraviolet wavelength, shedding new


00:00:58.320 --> 00:01:00.470
light on structures and processes in the


00:01:00.480 --> 00:01:02.510
galactic region surrounding our solar


00:01:02.520 --> 00:01:05.030
system. In fact, these new landmark


00:01:05.040 --> 00:01:07.109
observations are providing astronomers


00:01:07.119 --> 00:01:09.190
with their first clear view of the sky


00:01:09.200 --> 00:01:10.789
surrounding the solar system at these


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wavelengths, and they're revealing both


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new characteristics of that sky and


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refuting old ideas. The study's lead


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author Randy Gladston from the Southwest


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Research Institute says the new findings


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are showing hot interstellar gas bubbles


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like the one our solar systems embedded


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within may actually be regions of


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enhanced hydrogen gas emissions at


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wavelengths known as lyman alpha. Lyman


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alpha is a specific wavelength of


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ultraviolet light emitted and scattered


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by hydrogen atoms. It's especially


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useful to astronomers studying distant


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stars, galaxies, and the interstellar


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medium as it can help detect the


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composition, temperature, and movement


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of these distant objects. During its


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initial journey to Pluto, New Horizons


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collected baseline data about lime and


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alpha emissions using its Alice


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ultraviolet spectrograph. Spectrograph


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split light into various wavelengths of


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colors, and Alice specializes in the far


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ultraviolet wavelength band. After the


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spacecraft's primary flyby of the dwarf


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planet Pluto and its binary partner


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Sharon, scientists used Alice to make


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broader and more frequent surveys of


00:02:14.160 --> 00:02:16.470
lime and alpha emissions as new horizons


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traveled further from the sun. These


00:02:18.959 --> 00:02:20.869
surveys included an extensive set of


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scans mapping roughly 83% of the sky. To


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isolate emissions from the galaxy,


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astronomers modeled scattered solar


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limema alpha emissions and then


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subtracted them from the specttograph's


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data. The results indicate a roughly


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uniform background lime and alpha sky


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brightness 10 times stronger than what


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was expected from previous estimates.


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Gladston says the results point to the


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emission and scattering of lime and


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alpha photons by hydrogen atoms in the


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shell of a hot bubble known as surround


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our solar system nearby stars. That


00:02:51.360 --> 00:02:53.509
bubble was formed by nearby supernova


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events millions of years ago. The study


00:02:55.920 --> 00:02:57.910
also found no evidence that a hydrogen


00:02:57.920 --> 00:02:59.430
wall thought to surround the sun's


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heliosphere substantially contributes to


00:03:01.599 --> 00:03:03.910
the observed lime and alpha signal.


00:03:03.920 --> 00:03:05.830
Astronomers had theorized that a wall of


00:03:05.840 --> 00:03:07.430
interstellar hydrogen atoms would


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accumulate as they encountered the edge


00:03:09.360 --> 00:03:11.509
of the heliosphere. The vast region of


00:03:11.519 --> 00:03:13.750
space encapsulating our solar system


00:03:13.760 --> 00:03:16.390
dominated by the solar wind. However,


00:03:16.400 --> 00:03:18.470
the new horizon's data saw nothing to


00:03:18.480 --> 00:03:20.470
indicate the wall is an important source


00:03:20.480 --> 00:03:23.710
of lime and alpha emissions. This is


00:03:23.720 --> 00:03:26.550
spaceime still to come. Searching for


00:03:26.560 --> 00:03:29.110
the dark in the Martian light and NASA


00:03:29.120 --> 00:03:30.789
mission managers are investigating a


00:03:30.799 --> 00:03:32.309
major problem with the electric


00:03:32.319 --> 00:03:34.070
propulsion system aboard its Psyche


00:03:34.080 --> 00:03:36.149
spacecraft. All that and more still to


00:03:36.159 --> 00:03:38.120
come on


00:03:38.130 --> 00:03:40.190
[Music]


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Spaceime. This episode of Spacetime is


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brought to you by NordVPN, our official


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NordVPN. And now it's back to our show.


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[Music]


00:05:10.080 --> 00:05:12.230
NASA's Mars Perseverance rover has been


00:05:12.240 --> 00:05:14.070
busy over the past week continuing its


00:05:14.080 --> 00:05:15.909
exploration of the lower witch Hazel


00:05:15.919 --> 00:05:17.830
Hill outcrop exposed on the edge of the


00:05:17.840 --> 00:05:20.469
Jezro crater rim. The formations


00:05:20.479 --> 00:05:22.710
composed of alternating light and dark


00:05:22.720 --> 00:05:25.029
layers of rock and mission managers have


00:05:25.039 --> 00:05:26.710
been busy trying to understand the


00:05:26.720 --> 00:05:29.350
makeup and relationship of these layers.


00:05:29.360 --> 00:05:31.350
A few weeks ago, they sampled one of the


00:05:31.360 --> 00:05:33.110
light tone layers at a place they've


00:05:33.120 --> 00:05:35.189
named Maine River. They discovered it


00:05:35.199 --> 00:05:36.950
was made up of very small clasts or


00:05:36.960 --> 00:05:39.590
fragments of rocks and minerals. Since


00:05:39.600 --> 00:05:41.350
then, scientists have learned that the


00:05:41.360 --> 00:05:43.350
darker layers tend to be composed of


00:05:43.360 --> 00:05:45.430
larger classs compared to the lighter


00:05:45.440 --> 00:05:47.110
layers, and they've been searching for a


00:05:47.120 --> 00:05:49.110
place to sample this coarser grain rock


00:05:49.120 --> 00:05:51.510
type. Sometimes these coarser grain


00:05:51.520 --> 00:05:53.590
rocks also contain sphererals which are


00:05:53.600 --> 00:05:55.270
of great interest to scientists because


00:05:55.280 --> 00:05:56.950
they provide clues about the very


00:05:56.960 --> 00:05:58.790
processes that form the layered rock


00:05:58.800 --> 00:06:00.710
formations in the first place.


00:06:00.720 --> 00:06:02.629
Perseverance first looked at a dark


00:06:02.639 --> 00:06:05.189
layer at punchon rock using its abrasion


00:06:05.199 --> 00:06:07.749
tool. They then examined another dark


00:06:07.759 --> 00:06:09.350
layer at a formation known as wreck


00:06:09.360 --> 00:06:11.270
apple but couldn't find a suitable space


00:06:11.280 --> 00:06:14.230
to araid. So while scientists searched


00:06:14.240 --> 00:06:16.230
for other locations to study the coarse


00:06:16.240 --> 00:06:18.390
grain units and sphererals, Perseverance


00:06:18.400 --> 00:06:20.390
drove further south to a place known as


00:06:20.400 --> 00:06:23.029
Port Anson. Port Anson's intriguing


00:06:23.039 --> 00:06:25.110
because from orbit it showed a clear


00:06:25.120 --> 00:06:27.029
contact between the lighter layers of


00:06:27.039 --> 00:06:29.270
witch hazel hill and a distinct unit


00:06:29.280 --> 00:06:31.909
below it. And although the rocks below


00:06:31.919 --> 00:06:33.990
the poansen contact point do show


00:06:34.000 --> 00:06:35.430
interesting compositional differences


00:06:35.440 --> 00:06:37.029
with those of witch hazel hill, they


00:06:37.039 --> 00:06:38.230
weren't the coarse grain rocks


00:06:38.240 --> 00:06:40.469
scientists were looking for. Still, they


00:06:40.479 --> 00:06:42.629
did perform an abrasion test there at a


00:06:42.639 --> 00:06:44.550
location they've named Strong Island


00:06:44.560 --> 00:06:46.469
before driving back up north for what


00:06:46.479 --> 00:06:48.230
hopefully will be another attempt at


00:06:48.240 --> 00:06:51.029
investigating the coarser grain rocks.


00:06:51.039 --> 00:06:53.309
Needless to say, we'll keep you


00:06:53.319 --> 00:06:56.629
informed. This is Spaceime. Still to


00:06:56.639 --> 00:06:58.230
come, NASA mission managers


00:06:58.240 --> 00:07:00.150
investigating a serious problem with the


00:07:00.160 --> 00:07:01.909
electric propulsion system aboard its


00:07:01.919 --> 00:07:04.550
Psyche spacecraft. And we explore the


00:07:04.560 --> 00:07:06.950
constellation Scorpius, the spectacular


00:07:06.960 --> 00:07:09.909
M6 and M7 open star clusters, and the


00:07:09.919 --> 00:07:12.870
ETAs meteor shower produced by Hal's


00:07:12.880 --> 00:07:15.870
Comet in the May edition of Skywatch.


00:07:15.880 --> 00:07:23.080
[Music]




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NASA mission managers are investigating


00:07:32.160 --> 00:07:33.670
a problem with the electric propulsion


00:07:33.680 --> 00:07:36.230
system aboard the Saki spacecraft.


00:07:36.240 --> 00:07:37.990
Launched on a Falcon Heavy rocket back


00:07:38.000 --> 00:07:42.550
in October 2023, the 2,68 kg probe is on


00:07:42.560 --> 00:07:44.629
a mission to explore the metallic main


00:07:44.639 --> 00:07:47.270
belt asteroid 16 Psyche in order to


00:07:47.280 --> 00:07:49.189
learn more about the origins of


00:07:49.199 --> 00:07:52.629
planetary cores. 16 Sakis, the heaviest


00:07:52.639 --> 00:07:55.189
known Mtype asteroid, and it may be the


00:07:55.199 --> 00:07:57.670
exposed iron core of a protolanet, the


00:07:57.680 --> 00:07:59.270
remnant of a violent collision with


00:07:59.280 --> 00:08:01.350
another object that stripped this body


00:08:01.360 --> 00:08:04.070
off its metal and crust. The spacecraft


00:08:04.080 --> 00:08:06.629
will eventually spend 817 Earth days


00:08:06.639 --> 00:08:09.430
orbiting the strange 226 km wide


00:08:09.440 --> 00:08:11.830
metallic world. But it's got to get


00:08:11.840 --> 00:08:13.990
there first. Mission managers with


00:08:14.000 --> 00:08:15.670
NASA's Jet Propulsion Laboratory in


00:08:15.680 --> 00:08:17.830
Pasin, California, say the spacecraft's


00:08:17.840 --> 00:08:19.909
electric thrusters shut down on April


00:08:19.919 --> 00:08:21.990
the 1st when pressure fell in the line


00:08:22.000 --> 00:08:24.070
that feeds Xeon propellant to the Hall


00:08:24.080 --> 00:08:26.469
effect thrusters. The pressure dropped


00:08:26.479 --> 00:08:29.510
from 248 kilopascals down to 179,


00:08:29.520 --> 00:08:31.909
causing the thrusters to stop working.


00:08:31.919 --> 00:08:33.670
The probe turned on its hall effect


00:08:33.680 --> 00:08:36.389
thrusters in May 2024, which combined


00:08:36.399 --> 00:08:38.389
with a gravity assist Mars flyby


00:08:38.399 --> 00:08:40.230
scheduled for May next year will allow


00:08:40.240 --> 00:08:43.149
the probe to arrive at Psyche in August


00:08:43.159 --> 00:08:45.509
2029. Now, right now, there's not too


00:08:45.519 --> 00:08:47.750
much to worry about. Psyche can continue


00:08:47.760 --> 00:08:49.829
to coast until the middle of June before


00:08:49.839 --> 00:08:51.470
there's a significant effect on its


00:08:51.480 --> 00:08:53.430
trajectory. Right now, potential


00:08:53.440 --> 00:08:55.350
solutions include switching to a backup


00:08:55.360 --> 00:08:57.670
propellant line. It's the first major


00:08:57.680 --> 00:08:59.269
problem with the spacecraft which had


00:08:59.279 --> 00:09:00.949
been working normally since its long


00:09:00.959 --> 00:09:03.350
delayed launch. See, the project had


00:09:03.360 --> 00:09:04.870
suffered a series of development


00:09:04.880 --> 00:09:07.190
problems during its construction phase.


00:09:07.200 --> 00:09:09.509
These included the co pandemic and


00:09:09.519 --> 00:09:11.829
software testing delays which pushed


00:09:11.839 --> 00:09:13.430
back the launch date from the originally


00:09:13.440 --> 00:09:17.190
slated August 2022 by more than a year.


00:09:17.200 --> 00:09:23.330
This is spaceime


00:09:23.340 --> 00:09:35.110
[Music]


00:09:35.120 --> 00:09:36.870
And time now to turn our eyes to the


00:09:36.880 --> 00:09:38.790
skies and check out the celestial sphere


00:09:38.800 --> 00:09:42.150
for the month of May on Skywatch. May is


00:09:42.160 --> 00:09:43.829
the fifth month of the year in both the


00:09:43.839 --> 00:09:46.949
Julian and Gagorian calendars. The month


00:09:46.959 --> 00:09:49.350
was named for the Greek goddess Maya who


00:09:49.360 --> 00:09:51.269
was identified with the Roman era


00:09:51.279 --> 00:09:53.430
goddess of fertility Bonadia whose


00:09:53.440 --> 00:09:55.750
festival was held in May. But I guess


00:09:55.760 --> 00:09:57.110
more importantly for many of our


00:09:57.120 --> 00:09:59.350
listeners, May typically marks the start


00:09:59.360 --> 00:10:01.670
of summer vacation season in the United


00:10:01.680 --> 00:10:04.389
States and Canada. Let's start our tour


00:10:04.399 --> 00:10:06.550
of the night skies by looking east where


00:10:06.560 --> 00:10:08.389
you'll see the constellation Scorpius,


00:10:08.399 --> 00:10:11.190
the Scorpion. In Greek mythology, the


00:10:11.200 --> 00:10:13.190
constellation was named after Scorpius,


00:10:13.200 --> 00:10:14.790
who was sent to Earth by the goddess


00:10:14.800 --> 00:10:17.030
Gaia, in order to slay Orion, the


00:10:17.040 --> 00:10:18.949
Hunter, after he boasted that he could


00:10:18.959 --> 00:10:21.750
kill all the animals on Earth. Scorpius


00:10:21.760 --> 00:10:24.870
stung Orion in the shoulder. But Orion's


00:10:24.880 --> 00:10:27.670
life was spared by Ofious, the healer,


00:10:27.680 --> 00:10:29.430
and it was placed in the heavens along


00:10:29.440 --> 00:10:31.750
with Scorpius, who continues to pursue


00:10:31.760 --> 00:10:34.630
him for eternity. Orion the hunter has


00:10:34.640 --> 00:10:36.949
become the hunted forever with Scorpius


00:10:36.959 --> 00:10:39.030
rising in the east this time of year to


00:10:39.040 --> 00:10:41.350
triumphantly chase and defeat Orion who


00:10:41.360 --> 00:10:44.310
sets in the west. Meanwhile, Ofucius the


00:10:44.320 --> 00:10:46.069
healer rises in the east following


00:10:46.079 --> 00:10:48.470
behind Scorpius to chase and crush him


00:10:48.480 --> 00:10:50.630
into the earth as the scorpion sets in


00:10:50.640 --> 00:10:53.829
the west. And so this ancient story


00:10:53.839 --> 00:10:55.750
continues to play out in the heavens


00:10:55.760 --> 00:10:58.710
year after year. Interestingly, parts of


00:10:58.720 --> 00:11:01.430
the story predate the Greeks with Orion


00:11:01.440 --> 00:11:03.670
known in ancient Egypt as Osiris, the


00:11:03.680 --> 00:11:05.870
god of the underworld and of


00:11:05.880 --> 00:11:07.990
regeneration. The brightest star in


00:11:08.000 --> 00:11:10.870
Scorpius is Alpha Scorpio or Antares,


00:11:10.880 --> 00:11:13.350
the scorpion's heart. In ancient Greek,


00:11:13.360 --> 00:11:15.829
the name Antares means the equal arrival


00:11:15.839 --> 00:11:18.630
of Mars, the god of war. That's because


00:11:18.640 --> 00:11:20.790
its golden orange appearance is similar


00:11:20.800 --> 00:11:22.949
to that of the red planet, and it passes


00:11:22.959 --> 00:11:26.630
very close to Mars every 780 years.


00:11:26.640 --> 00:11:28.790
easily seen with the unaded eye and


00:11:28.800 --> 00:11:32.069
Tares is some 550 lighty years away but


00:11:32.079 --> 00:11:34.670
it looks so bright because it's around


00:11:34.680 --> 00:11:37.750
57,500 times as luminous as the sun and


00:11:37.760 --> 00:11:40.269
is one of the largest known stars in the


00:11:40.279 --> 00:11:44.230
universe. Ant is a red super giant about


00:11:44.240 --> 00:11:47.110
18 times the mass and 883 times the


00:11:47.120 --> 00:11:49.829
diameter of the sun. Were it placed


00:11:49.839 --> 00:11:51.990
where the sun is in our solar system, it


00:11:52.000 --> 00:11:53.590
would engulf all the terrestrial


00:11:53.600 --> 00:11:55.590
planets, Mercury, Venus, Earth, and


00:11:55.600 --> 00:11:57.910
Mars. And its visible surface would


00:11:57.920 --> 00:12:00.949
extend almost as far out as Jupiter. A


00:12:00.959 --> 00:12:02.630
lightyear is about 10 trillion


00:12:02.640 --> 00:12:04.949
kilometers. The distance a photon can


00:12:04.959 --> 00:12:08.310
travel in a year at 300,000 km/s, the


00:12:08.320 --> 00:12:10.150
speed of light in a vacuum, and the


00:12:10.160 --> 00:12:12.710
ultimate speed limit of the universe.


00:12:12.720 --> 00:12:15.110
Astronomers believe Antaris began life


00:12:15.120 --> 00:12:17.110
around 12 million years ago as a


00:12:17.120 --> 00:12:19.829
spectrotype O or B blue star.


00:12:19.839 --> 00:12:22.150
Astronomers describe stars in terms of


00:12:22.160 --> 00:12:24.389
spectral types, a classification system


00:12:24.399 --> 00:12:25.870
based on temperature and


00:12:25.880 --> 00:12:27.829
characteristics. The hottest, most


00:12:27.839 --> 00:12:29.910
massive, and most luminous stars are


00:12:29.920 --> 00:12:32.710
known as spectrotype O blue stars.


00:12:32.720 --> 00:12:34.710
They're followed by spectrotype B blue


00:12:34.720 --> 00:12:37.269
white stars. Then spectrotype A white


00:12:37.279 --> 00:12:39.829
stars, spectrotype F whitish yellow


00:12:39.839 --> 00:12:42.550
stars, spectrotype G yellow stars.


00:12:42.560 --> 00:12:44.230
That's where our sun fits in. Then


00:12:44.240 --> 00:12:46.790
there's spectrotype K orange stars. And


00:12:46.800 --> 00:12:48.949
the coolest and least massive stars are


00:12:48.959 --> 00:12:52.069
known as spectrotype M red stars. Each


00:12:52.079 --> 00:12:54.069
spectral classification system can also


00:12:54.079 --> 00:12:56.550
be subdivided using a numeric digit to


00:12:56.560 --> 00:12:58.389
represent temperature with zero being


00:12:58.399 --> 00:13:01.190
the hottest and nine the coolest. And


00:13:01.200 --> 00:13:02.870
then you add a Roman numeral to


00:13:02.880 --> 00:13:05.509
represent luminosity. So put it all


00:13:05.519 --> 00:13:07.829
together and you can describe our sun as


00:13:07.839 --> 00:13:12.470
being a G2V or G25 yellow dwarf star,


00:13:12.480 --> 00:13:14.910
one of millions spread across our


00:13:14.920 --> 00:13:17.269
galaxy. Also included in the stellar


00:13:17.279 --> 00:13:19.430
classification system are special types


00:13:19.440 --> 00:13:21.829
LT and Y which are assigned to failed


00:13:21.839 --> 00:13:24.069
stars known as brown dwarves. Some of


00:13:24.079 --> 00:13:25.990
which were actually born as spectrotype


00:13:26.000 --> 00:13:28.550
M red stars but became brown dwarves


00:13:28.560 --> 00:13:31.030
after losing some of their mass. Brown


00:13:31.040 --> 00:13:33.030
dwarves fit into a unique category


00:13:33.040 --> 00:13:34.629
between the largest planets, which are


00:13:34.639 --> 00:13:36.710
about 13 times the mass of Jupiter, and


00:13:36.720 --> 00:13:38.870
the smallest spectrotype M red dwarf


00:13:38.880 --> 00:13:41.430
stars, which are about 75 to 80 times


00:13:41.440 --> 00:13:44.990
the mass of Jupiter, or 0.08 solar


00:13:45.000 --> 00:13:47.750
masses. Like the similarsized red giant


00:13:47.760 --> 00:13:50.150
Betalers in the constellation Orion,


00:13:50.160 --> 00:13:52.230
Antares will almost certainly end its


00:13:52.240 --> 00:13:54.870
life as a spectacular type 2 or core


00:13:54.880 --> 00:13:57.350
collapse supernova, probably sometime


00:13:57.360 --> 00:13:59.910
within the next 100,000 years or so.


00:13:59.920 --> 00:14:01.750
When it does explode, it'll appear as


00:14:01.760 --> 00:14:03.509
bright as the full moon for several


00:14:03.519 --> 00:14:05.670
months on end and will be clearly


00:14:05.680 --> 00:14:07.750
visible during daylight hours here on


00:14:07.760 --> 00:14:10.550
Earth. Antares has a companion star,


00:14:10.560 --> 00:14:15.110
Antares B, located between 224 and 529


00:14:15.120 --> 00:14:16.870
astronomical units away from the


00:14:16.880 --> 00:14:19.430
primary. An astronomical unit is the


00:14:19.440 --> 00:14:21.030
average distance between the Earth and


00:14:21.040 --> 00:14:23.350
the Sun, which is about 150 million


00:14:23.360 --> 00:14:27.189
kilome or 8.3 light minutes. Spectral


00:14:27.199 --> 00:14:29.750
analysis of Antares B indicates it's


00:14:29.760 --> 00:14:31.269
pulling a lot of material off its


00:14:31.279 --> 00:14:33.629
bloated red super giant


00:14:33.639 --> 00:14:36.870
companion. Located near Antares is the


00:14:36.880 --> 00:14:40.150
M4 globular cluster. Globular clusters


00:14:40.160 --> 00:14:42.150
are tight balls densely packed with


00:14:42.160 --> 00:14:44.310
thousands to millions of stars which


00:14:44.320 --> 00:14:46.389
were either all originally formed at the


00:14:46.399 --> 00:14:47.990
same time from the collapse of the same


00:14:48.000 --> 00:14:49.990
molecular gas and dust cloud or


00:14:50.000 --> 00:14:52.310
alternatively their galactic centers.


00:14:52.320 --> 00:14:54.150
the remains of ancient galaxies that


00:14:54.160 --> 00:14:55.750
have been merged into the Milky Way


00:14:55.760 --> 00:14:59.269
galaxy over billions of years. M4 is


00:14:59.279 --> 00:15:01.110
composed of a million or so stars


00:15:01.120 --> 00:15:03.269
originally born some 12 billion years


00:15:03.279 --> 00:15:06.550
ago. The M4 globular cluster is located


00:15:06.560 --> 00:15:09.509
some 7,200 light years away, making it


00:15:09.519 --> 00:15:11.310
one of the nearest globular clusters to


00:15:11.320 --> 00:15:13.829
Earth. Easily seen through a pair of


00:15:13.839 --> 00:15:16.069
small binoculars, it covers an area of


00:15:16.079 --> 00:15:18.470
the sky as seen from Earth as big as the


00:15:18.480 --> 00:15:21.030
full moon. Astronomers estimate there


00:15:21.040 --> 00:15:23.829
are some 150 or so globular clusters


00:15:23.839 --> 00:15:26.189
orbiting in the halo of the Milky


00:15:26.199 --> 00:15:28.790
Way. Located near the tail of the


00:15:28.800 --> 00:15:31.189
scorpion are two open star clusters


00:15:31.199 --> 00:15:34.710
known as M6 and M7. Open star clusters


00:15:34.720 --> 00:15:36.389
are loosely bound groups of a few


00:15:36.399 --> 00:15:38.550
thousand stars which all originally


00:15:38.560 --> 00:15:40.389
formed from the same molecular gas and


00:15:40.399 --> 00:15:42.470
dust cloud at the same time but are not


00:15:42.480 --> 00:15:45.350
as densely bound as globular clusters.


00:15:45.360 --> 00:15:47.189
Open clusters generally survive for a


00:15:47.199 --> 00:15:49.030
few hundred million years with the most


00:15:49.040 --> 00:15:50.870
massive ones surviving for maybe a few


00:15:50.880 --> 00:15:53.590
billion years. Now, in contrast, the far


00:15:53.600 --> 00:15:56.150
more massive globular clusters exert far


00:15:56.160 --> 00:15:57.990
stronger gravitational attraction on


00:15:58.000 --> 00:15:59.590
their members, which is why they can


00:15:59.600 --> 00:16:02.389
survive so much longer. M6, which is


00:16:02.399 --> 00:16:04.389
also known as the butterfly cluster, is


00:16:04.399 --> 00:16:06.870
some 12 light years across and located


00:16:06.880 --> 00:16:09.430
about 1,600 lighty years away. It


00:16:09.440 --> 00:16:11.430
contains around 80 stars which are all


00:16:11.440 --> 00:16:13.590
less than 100 million years old which is


00:16:13.600 --> 00:16:17.189
quite young in cosmic terms. The M7 or


00:16:17.199 --> 00:16:19.590
Tom cluster is named after the famous


00:16:19.600 --> 00:16:21.189
Greek astronomer and mathematician


00:16:21.199 --> 00:16:24.710
Claudius Tom. It's about 980 light years


00:16:24.720 --> 00:16:27.509
away and is far more dispersed than M6


00:16:27.519 --> 00:16:29.870
covering an area around 25 lighty years


00:16:29.880 --> 00:16:32.949
across. And at around 200 million years,


00:16:32.959 --> 00:16:35.590
it's about twice as old.


00:16:35.600 --> 00:16:39.030
By the way, the M in terms like M4, M6,


00:16:39.040 --> 00:16:42.470
and M7 are abbreviations for Messier in


00:16:42.480 --> 00:16:43.910
honor of the 18th century French


00:16:43.920 --> 00:16:45.590
astronomer Charles Messier, who


00:16:45.600 --> 00:16:47.670
developed an astronomical catalog of


00:16:47.680 --> 00:16:50.629
fuzzy, nebulous objects in the skies.


00:16:50.639 --> 00:16:53.269
See, Messier was a comet hunter, and he


00:16:53.279 --> 00:16:55.990
compiled a list of 103 fuzzy objects


00:16:56.000 --> 00:16:58.150
which weren't comets, and so from his


00:16:58.160 --> 00:17:00.790
perspective could be ignored. Later,


00:17:00.800 --> 00:17:02.470
other astronomers added additional


00:17:02.480 --> 00:17:04.390
celestial objects to the list, bringing


00:17:04.400 --> 00:17:06.510
the present catalog up to


00:17:06.520 --> 00:17:09.669
110. Our solar system, in fact, most of


00:17:09.679 --> 00:17:11.510
the stars we see when we look up in the


00:17:11.520 --> 00:17:13.909
night sky, are located in the Milky Way


00:17:13.919 --> 00:17:17.429
galaxy's Orion arm. The Orion arm, also


00:17:17.439 --> 00:17:19.590
known as the Orion spur or the Orion


00:17:19.600 --> 00:17:21.590
Signis arm, depending on which name you


00:17:21.600 --> 00:17:24.710
prefer, is some 3,500 lighty years wide


00:17:24.720 --> 00:17:27.829
and around 10,000 lighty years long. The


00:17:27.839 --> 00:17:30.110
Orion arm is named after the Orion


00:17:30.120 --> 00:17:31.990
constellation which is one of the most


00:17:32.000 --> 00:17:33.830
prominent constellations in the southern


00:17:33.840 --> 00:17:35.350
hemisphere summer and northern


00:17:35.360 --> 00:17:37.990
hemisphere winter. Some of the brightest


00:17:38.000 --> 00:17:40.150
and most famous celestial objects in the


00:17:40.160 --> 00:17:43.350
constellation include bettle riel the


00:17:43.360 --> 00:17:45.750
stars of the Orion belt and the Orion


00:17:45.760 --> 00:17:48.789
nebula all located within the Orion arm.


00:17:48.799 --> 00:17:50.789
The Orion arm is located between the


00:17:50.799 --> 00:17:53.029
Karina Sagittarius arm which is more


00:17:53.039 --> 00:17:54.710
towards the galactic center from our


00:17:54.720 --> 00:17:57.029
position and the Perseus arm which is


00:17:57.039 --> 00:17:58.470
more towards the outer edge of the


00:17:58.480 --> 00:18:00.390
galaxy from our point of view. The


00:18:00.400 --> 00:18:02.710
Perseus arm is one of the two major arms


00:18:02.720 --> 00:18:04.789
of the Milky Way. The other being the


00:18:04.799 --> 00:18:07.830
Scutum Centurus arm. Long thought of as


00:18:07.840 --> 00:18:10.470
a minor structure, a spur if you will


00:18:10.480 --> 00:18:12.549
between the two longer adjacent arms,


00:18:12.559 --> 00:18:15.190
Perseus and Karina Sagittarius. Evidence


00:18:15.200 --> 00:18:17.909
was presented in mid 2013 that the Orion


00:18:17.919 --> 00:18:19.590
arm might actually be a branch of the


00:18:19.600 --> 00:18:21.830
Perseus arm or possibly a completely


00:18:21.840 --> 00:18:24.549
independent arm segment itself. Within


00:18:24.559 --> 00:18:27.190
the Orion arm, our solar system, the


00:18:27.200 --> 00:18:28.549
sun, the Earth, and all the other


00:18:28.559 --> 00:18:30.630
planets we know are located close to the


00:18:30.640 --> 00:18:32.870
inner rim in what's known as the local


00:18:32.880 --> 00:18:35.270
bubble. About halfway along the Orion


00:18:35.280 --> 00:18:37.830
arm's length, approximately 26,000 light


00:18:37.840 --> 00:18:40.230
years from the galactic center. The


00:18:40.240 --> 00:18:42.070
local bubble is a cavity in the


00:18:42.080 --> 00:18:44.070
interstellar medium in the Orion arm


00:18:44.080 --> 00:18:45.909
containing among other things the local


00:18:45.919 --> 00:18:47.830
interstellar cloud which contains our


00:18:47.840 --> 00:18:50.870
solar system and the G-Cloud. It's at


00:18:50.880 --> 00:18:53.669
least 300 light years across and it has


00:18:53.679 --> 00:18:56.950
a neutral hydrogen density of just 0.05


00:18:56.960 --> 00:18:59.830
atoms per cm. That's just 1/10enth of


00:18:59.840 --> 00:19:01.590
the average for the interstellar medium


00:19:01.600 --> 00:19:03.990
across the Milky Way and about a sixth


00:19:04.000 --> 00:19:06.310
that of the local interstellar cloud.


00:19:06.320 --> 00:19:08.470
The hot diffused gas in the local bubble


00:19:08.480 --> 00:19:10.710
emits X-rays and is the result of a


00:19:10.720 --> 00:19:12.870
supernova that exploded sometime during


00:19:12.880 --> 00:19:15.750
the past 10 to 20 million years. It was


00:19:15.760 --> 00:19:17.270
once thought that the most likely


00:19:17.280 --> 00:19:18.630
candidate for the remains of this


00:19:18.640 --> 00:19:21.350
supernova was Jiminga, a pulsar in the


00:19:21.360 --> 00:19:24.390
constellation Gemini. However, later it


00:19:24.400 --> 00:19:26.789
was suggested that modable supernova in


00:19:26.799 --> 00:19:29.270
a subgroup B1 of the Plleades moving


00:19:29.280 --> 00:19:31.350
group was more likely responsible


00:19:31.360 --> 00:19:33.990
becoming a remnant super shell. Our


00:19:34.000 --> 00:19:35.590
solar system has been traveling through


00:19:35.600 --> 00:19:37.590
this region of space occupied by the


00:19:37.600 --> 00:19:39.750
local bubble for the last 5 to 10


00:19:39.760 --> 00:19:42.710
million years. Its current location is


00:19:42.720 --> 00:19:43.990
in what's known as the local


00:19:44.000 --> 00:19:46.710
interstellar cloud. A minor region of


00:19:46.720 --> 00:19:48.549
slightly denser material within the


00:19:48.559 --> 00:19:50.950
bubble. The cloud formed when the local


00:19:50.960 --> 00:19:52.789
bubble and another bubble called the


00:19:52.799 --> 00:19:55.590
loop one bubble met. Gas within the


00:19:55.600 --> 00:19:57.510
local interstellar cloud has a density


00:19:57.520 --> 00:20:01.350
of about 0.3 atoms per cm. From what we


00:20:01.360 --> 00:20:02.870
can tell, the local bubble isn't


00:20:02.880 --> 00:20:05.190
spherical, but seems to be narrower in


00:20:05.200 --> 00:20:07.270
the galactic plane, becoming somewhat


00:20:07.280 --> 00:20:09.430
egg- shaped or elliptical, and may even


00:20:09.440 --> 00:20:11.029
become wider above and below the


00:20:11.039 --> 00:20:13.190
galactic plane, becoming shaped more


00:20:13.200 --> 00:20:15.830
like an hourglass. And it's not alone.


00:20:15.840 --> 00:20:17.990
It's abuting other bubbles of lesser


00:20:18.000 --> 00:20:20.150
dense interstellar medium, including the


00:20:20.160 --> 00:20:22.710
loop one bubble. The loop one bubble was


00:20:22.720 --> 00:20:25.029
created by supernova and stellar winds


00:20:25.039 --> 00:20:27.270
in the Scorpio Centurus Association,


00:20:27.280 --> 00:20:29.990
some 500 light years from the sun. The


00:20:30.000 --> 00:20:32.070
loop one bubble also contains the star


00:20:32.080 --> 00:20:34.789
antures that we spoke about earlier.


00:20:34.799 --> 00:20:36.950
Astronomers have identified several well


00:20:36.960 --> 00:20:38.870
I guess you'd call them tunnels which


00:20:38.880 --> 00:20:40.789
connect the cavities of the local bubble


00:20:40.799 --> 00:20:42.710
with that of the loop one bubble.


00:20:42.720 --> 00:20:44.390
Collectively they've been referred to as


00:20:44.400 --> 00:20:46.630
the lupus tunnel. Other bubbles which


00:20:46.640 --> 00:20:48.470
are adjacent to our local bubble and


00:20:48.480 --> 00:20:50.630
known as the loop 2 bubble and the loop


00:20:50.640 --> 00:20:52.870
three bubble. Looks like astronomers


00:20:52.880 --> 00:20:54.470
still have a problem when it comes to


00:20:54.480 --> 00:20:56.710
thinking up cool names.


00:20:56.720 --> 00:20:58.710
Also visible this month is the ETA


00:20:58.720 --> 00:21:01.270
awards meteor shower which is generated


00:21:01.280 --> 00:21:03.029
as the Earth passes through the dust and


00:21:03.039 --> 00:21:05.990
debris trail left behind by Hal's comet.


00:21:06.000 --> 00:21:08.630
Comet P1's a well-known short period


00:21:08.640 --> 00:21:10.310
comet which visits the inner solar


00:21:10.320 --> 00:21:14.310
system every 75 to 76 years. The 15


00:21:14.320 --> 00:21:16.390
kilometer wide mountain of rock and ice


00:21:16.400 --> 00:21:18.230
will make its next close-up appearance


00:21:18.240 --> 00:21:20.230
in 2061.


00:21:20.240 --> 00:21:21.830
It's named in honor of the British


00:21:21.840 --> 00:21:25.029
astronomer Edmund Halley who in 1705


00:21:25.039 --> 00:21:26.870
after examining ancient Chinese,


00:21:26.880 --> 00:21:28.950
Babylonian, and medieval European


00:21:28.960 --> 00:21:30.870
records successfully predicted its


00:21:30.880 --> 00:21:32.190
return in


00:21:32.200 --> 00:21:36.149
1758. However, he died in 1742 before


00:21:36.159 --> 00:21:38.549
his prediction could be confirmed. The


00:21:38.559 --> 00:21:40.630
comet's highly elliptical and elongated


00:21:40.640 --> 00:21:42.549
orbit takes it from between the orbits


00:21:42.559 --> 00:21:44.789
of Mercury and Venus out almost as far


00:21:44.799 --> 00:21:47.510
as the orbit of Pluto. Hali's orbit is


00:21:47.520 --> 00:21:49.830
in retrograde, meaning it orbits the sun


00:21:49.840 --> 00:21:51.430
in the opposite direction to the


00:21:51.440 --> 00:21:53.669
planets, that is clockwise from above


00:21:53.679 --> 00:21:56.390
the sun's northern pole. This retrograde


00:21:56.400 --> 00:21:58.070
orbit results in it having one of the


00:21:58.080 --> 00:21:59.990
highest velocities relative to the Earth


00:22:00.000 --> 00:22:02.070
of any object in the solar system,


00:22:02.080 --> 00:22:06.230
traveling at some 70.56 km/s, or if you


00:22:06.240 --> 00:22:08.190
prefer,


00:22:08.200 --> 00:22:11.510
254,016 km hour, as well as the


00:22:11.520 --> 00:22:14.310
Etoacrids meteor shower every May. Hal's


00:22:14.320 --> 00:22:16.789
comet also produces the Orionids meteor


00:22:16.799 --> 00:22:19.350
shower in late October. Astronomers


00:22:19.360 --> 00:22:21.510
think comet Halley was originally a long


00:22:21.520 --> 00:22:23.510
period comet which took thousands of


00:22:23.520 --> 00:22:25.110
years to travel to the inner solar


00:22:25.120 --> 00:22:27.190
system from the ought cloud but was


00:22:27.200 --> 00:22:28.950
gravitationally perturbed into its


00:22:28.960 --> 00:22:30.950
current orbit by close encounters with


00:22:30.960 --> 00:22:33.990
the giant outer planets. The cloud is a


00:22:34.000 --> 00:22:36.310
hypothetical sphere of comets and


00:22:36.320 --> 00:22:38.710
asteroids beyond the heliosphere. a


00:22:38.720 --> 00:22:40.630
mixture of vagabonds from the solar


00:22:40.640 --> 00:22:43.029
system and objects from deep space which


00:22:43.039 --> 00:22:44.470
have been collected by the sun's


00:22:44.480 --> 00:22:47.029
gravitational pole. Occasionally, as the


00:22:47.039 --> 00:22:49.510
sun passes by another star, an orcloud


00:22:49.520 --> 00:22:51.590
object will get perturbed and be flung


00:22:51.600 --> 00:22:54.070
towards the inner solar system. The


00:22:54.080 --> 00:22:56.470
Acrid's meteor shower runs from the 19th


00:22:56.480 --> 00:22:59.110
of April through to the 28th of May,


00:22:59.120 --> 00:23:01.430
peaking around May the 5th with around


00:23:01.440 --> 00:23:04.149
55 meteors an hour, making it one of the


00:23:04.159 --> 00:23:05.990
southern hemisphere's best celestial


00:23:06.000 --> 00:23:09.750
showers. However, back in 1975, they


00:23:09.760 --> 00:23:12.789
were running 95 meteors an hour. And in


00:23:12.799 --> 00:23:16.390
1980, it was up to 110. Even better, the


00:23:16.400 --> 00:23:18.390
bright yellow meteors often appear as


00:23:18.400 --> 00:23:21.270
streaks known as trains. As their name


00:23:21.280 --> 00:23:23.590
suggests, they radiate out from the


00:23:23.600 --> 00:23:25.430
direction of the constellation Aquarius


00:23:25.440 --> 00:23:27.990
and the star Eta Aquiry. Just look


00:23:28.000 --> 00:23:29.590
towards the east after midnight and


00:23:29.600 --> 00:23:32.470
before dawn for the best view. And


00:23:32.480 --> 00:23:34.230
joining us now for the rest of our tour


00:23:34.240 --> 00:23:36.549
of the May night skies and skywatch is


00:23:36.559 --> 00:23:38.630
science writer Jonathan Alli. Good day


00:23:38.640 --> 00:23:40.710
Stuart. Yes, it's May. So the nights are


00:23:40.720 --> 00:23:42.230
definitely getting longer and colder in


00:23:42.240 --> 00:23:43.750
the part of the planet where I live as


00:23:43.760 --> 00:23:45.350
we head towards winter. But you know


00:23:45.360 --> 00:23:46.630
despite the cold, this is actually a


00:23:46.640 --> 00:23:48.230
great time for stargazing if you live


00:23:48.240 --> 00:23:49.750
where I am in the southern hemisphere as


00:23:49.760 --> 00:23:51.669
there are lots of great southern


00:23:51.679 --> 00:23:53.750
constellations visible. So some of the


00:23:53.760 --> 00:23:54.870
ones that you know you got to be far


00:23:54.880 --> 00:23:57.029
south to see such as the southern cross


00:23:57.039 --> 00:23:58.470
which at the moment is standing pretty


00:23:58.480 --> 00:24:00.549
much upright high in the south in the


00:24:00.559 --> 00:24:02.149
middle part of the evening to its left


00:24:02.159 --> 00:24:03.909
we've got these two bright stars in the


00:24:03.919 --> 00:24:06.070
constellation centurus that's alpha and


00:24:06.080 --> 00:24:08.310
beta centuri and astronomers call them


00:24:08.320 --> 00:24:10.310
the two pointers because if you draw an


00:24:10.320 --> 00:24:11.909
imaginary line between them and then


00:24:11.919 --> 00:24:13.510
keep the line going it more or less


00:24:13.520 --> 00:24:15.350
points towards the southern cross. Those


00:24:15.360 --> 00:24:16.950
two stars are really quite bright and


00:24:16.960 --> 00:24:18.390
prominent and they're close together. So


00:24:18.400 --> 00:24:20.390
people often spot them before they spot


00:24:20.400 --> 00:24:21.830
the southern cross. Yeah, I was using


00:24:21.840 --> 00:24:23.350
them as a marker to help me find the


00:24:23.360 --> 00:24:24.710
southern cross. Yeah. Yeah. And look,


00:24:24.720 --> 00:24:26.070
they're they're very bright compared to


00:24:26.080 --> 00:24:28.070
the the star. The stars in Southern


00:24:28.080 --> 00:24:30.549
Cross are not particularly dim, but it's


00:24:30.559 --> 00:24:32.710
a small constellation and when people go


00:24:32.720 --> 00:24:34.710
out try to find the southern cross, they


00:24:34.720 --> 00:24:35.990
um they're looking for something bigger.


00:24:36.000 --> 00:24:37.430
So, they don't really notice the cross


00:24:37.440 --> 00:24:38.710
at first. So, if you find these two


00:24:38.720 --> 00:24:39.990
pointer stars and then you just draw


00:24:40.000 --> 00:24:41.669
this do this trick of drawing the line


00:24:41.679 --> 00:24:43.110
and extending it a bit, then you think,


00:24:43.120 --> 00:24:44.470
"Oh, that's the southern that crosses


00:24:44.480 --> 00:24:46.149
it." So, uh yeah, they're very they're


00:24:46.159 --> 00:24:47.830
quite handy. Now, in the vicinity of the


00:24:47.840 --> 00:24:49.110
cross, there are two interesting sites


00:24:49.120 --> 00:24:50.710
to see, although you probably do need


00:24:50.720 --> 00:24:54.149
some non city dark skies to get a good


00:24:54.159 --> 00:24:55.350
view of them. The first of them is


00:24:55.360 --> 00:24:57.669
what's called the Cold Sack Nebula,


00:24:57.679 --> 00:24:59.830
which is a dark patch in the Milky Way


00:24:59.840 --> 00:25:01.190
right next to the Southern Cross. It's


00:25:01.200 --> 00:25:02.549
quite large. It's It's Yeah, it's


00:25:02.559 --> 00:25:03.909
probably about half the size or more of


00:25:03.919 --> 00:25:05.430
the Southern Cross. Yeah, this is quite


00:25:05.440 --> 00:25:07.510
large actually. It's a huge cloud of gas


00:25:07.520 --> 00:25:10.470
and dust almost 600 light years away.


00:25:10.480 --> 00:25:12.390
And because it's a very thick cloud of


00:25:12.400 --> 00:25:13.990
gas and dust, it's blocking out the


00:25:14.000 --> 00:25:16.390
light of the stars behind it. So, um,


00:25:16.400 --> 00:25:17.990
you know, years and years and years ago


00:25:18.000 --> 00:25:19.669
before photography started to come


00:25:19.679 --> 00:25:21.590
along, astronomers weren't really sure


00:25:21.600 --> 00:25:23.990
was this was this a hole in the Milky


00:25:24.000 --> 00:25:25.190
Way, and we're looking straight through


00:25:25.200 --> 00:25:28.470
to out to the other side, or is this a


00:25:28.480 --> 00:25:30.149
big dark something that's blocking the


00:25:30.159 --> 00:25:32.390
light from the stars behind? And yes, it


00:25:32.400 --> 00:25:35.190
is a big dark blob that is blocking the


00:25:35.200 --> 00:25:36.549
light of the stars behind it. There are


00:25:36.559 --> 00:25:38.149
stars in front of it, too, but not too


00:25:38.159 --> 00:25:40.149
many. They're not very um obvious to the


00:25:40.159 --> 00:25:42.070
naked eye. But you probably do need dark


00:25:42.080 --> 00:25:44.390
stars to see the um the Colac Nebula. I


00:25:44.400 --> 00:25:46.310
struggle to see it from where I am in


00:25:46.320 --> 00:25:48.230
suburbia. The other object of interest


00:25:48.240 --> 00:25:50.230
is a small star cluster called the jewel


00:25:50.240 --> 00:25:52.630
box, which is located a bit below and to


00:25:52.640 --> 00:25:54.789
the left of the leftmost star in the


00:25:54.799 --> 00:25:56.630
southern cross. Now, if you live in the


00:25:56.640 --> 00:25:58.149
city, you might just be able to make it


00:25:58.159 --> 00:25:59.669
out with your own eyes, but a pair of


00:25:59.679 --> 00:26:01.510
binoculars will definitely help. And


00:26:01.520 --> 00:26:02.950
through them, you'll see a pretty


00:26:02.960 --> 00:26:05.669
collection, maybe half a dozen, seven or


00:26:05.679 --> 00:26:07.750
eight, 10 stars perhaps, of different


00:26:07.760 --> 00:26:09.269
colors. That's why it's called a jewel


00:26:09.279 --> 00:26:10.950
box. And they're all closely packed


00:26:10.960 --> 00:26:12.630
together. All up, there are actually


00:26:12.640 --> 00:26:14.470
about a hundred stars in this cluster,


00:26:14.480 --> 00:26:15.590
but you're not going to see all of those


00:26:15.600 --> 00:26:17.110
with a pair of binoculars. You need big


00:26:17.120 --> 00:26:18.870
telescope to start see dozens and dozens


00:26:18.880 --> 00:26:20.470
of them. But it is really, really pretty


00:26:20.480 --> 00:26:21.990
and it's quite an easy one to see and


00:26:22.000 --> 00:26:23.830
it's fairly bright as star clusters go.


00:26:23.840 --> 00:26:25.149
That's much further away than the


00:26:25.159 --> 00:26:27.590
Colac's about 600 lighty years away.


00:26:27.600 --> 00:26:29.750
This little jewel box cluster is 6 and a


00:26:29.760 --> 00:26:32.310
half thousand light years away. Now to


00:26:32.320 --> 00:26:33.669
the right of the southern cross, as we


00:26:33.679 --> 00:26:35.110
look down to the south, you've got three


00:26:35.120 --> 00:26:36.870
large constellations. You've got Karina,


00:26:36.880 --> 00:26:39.029
VA, and Papus. all part of the Milky Way


00:26:39.039 --> 00:26:40.950
and they're full of glorious starfields


00:26:40.960 --> 00:26:42.870
and lots of nebulan things, including


00:26:42.880 --> 00:26:44.950
one called the Great Nebula in Karina.


00:26:44.960 --> 00:26:47.430
Now, this one rivals or in some people's


00:26:47.440 --> 00:26:50.630
opinions even exceed the splendor of the


00:26:50.640 --> 00:26:53.190
more famous nebula, the Orion Nebula,


00:26:53.200 --> 00:26:55.430
which is very easy to to make out


00:26:55.440 --> 00:26:57.029
because, you know, you can you need to


00:26:57.039 --> 00:26:58.630
see you need to be down south here to


00:26:58.640 --> 00:27:00.390
see the Karina. You got to be down south


00:27:00.400 --> 00:27:02.870
and it is a large fuzzy patch which you


00:27:02.880 --> 00:27:04.710
can see with your own eyes if you're


00:27:04.720 --> 00:27:06.710
under dark skies. But if you can get a


00:27:06.720 --> 00:27:08.630
telescope onto this region, uh, it just


00:27:08.640 --> 00:27:10.789
lets you see so much more. It really is


00:27:10.799 --> 00:27:13.269
is quite spectacular. It the extent of


00:27:13.279 --> 00:27:14.950
it, if you were able to see the whole


00:27:14.960 --> 00:27:16.470
thing with your just with your own eyes,


00:27:16.480 --> 00:27:18.310
it would be, you know, several times the


00:27:18.320 --> 00:27:20.630
width of the full moon. It's it's very


00:27:20.640 --> 00:27:22.390
large in the night sky. We don't notice


00:27:22.400 --> 00:27:25.669
it normally because it is fuzzy and


00:27:25.679 --> 00:27:28.390
faint. And most of us live in light


00:27:28.400 --> 00:27:31.909
polluted cities. So you you've got


00:27:31.919 --> 00:27:33.750
Buckley's chance as we say in Australia


00:27:33.760 --> 00:27:36.549
of seeing anything like this from light


00:27:36.559 --> 00:27:38.149
polluted light polluted skies. So you


00:27:38.159 --> 00:27:39.990
need to get somewhere dark and let your


00:27:40.000 --> 00:27:42.390
eyes get dark adapted. Now in the nearby


00:27:42.400 --> 00:27:44.149
constellation, same sort of well the


00:27:44.159 --> 00:27:45.549
other side of the cross really got


00:27:45.559 --> 00:27:47.909
centurus. You can find the globular star


00:27:47.919 --> 00:27:49.909
cluster Omega Centuri. Now this one is


00:27:49.919 --> 00:27:52.470
quite easy to see. It's visible as a


00:27:52.480 --> 00:27:54.950
just a what looks like a fuzgy star to


00:27:54.960 --> 00:27:57.029
the unaded eye. You got a pair of


00:27:57.039 --> 00:27:58.950
binoculars. It'll it'll reveal it


00:27:58.960 --> 00:27:59.750
depending on the size of your


00:27:59.760 --> 00:28:01.269
binoculars. It should reveal it to be


00:28:01.279 --> 00:28:04.870
like a small gray ball, just a tiny gray


00:28:04.880 --> 00:28:07.669
ball, but a telescope will show its true


00:28:07.679 --> 00:28:10.630
nature, which is a huge globe of


00:28:10.640 --> 00:28:13.029
seemingly countless stars, a globular


00:28:13.039 --> 00:28:14.789
star cluster, it's called it's called.


00:28:14.799 --> 00:28:16.789
It's an really impressive site. And if


00:28:16.799 --> 00:28:19.110
you get on the internet and have a look


00:28:19.120 --> 00:28:21.990
for Omega Centuri, you'll see what I


00:28:22.000 --> 00:28:23.830
mean. It is the most in fact, it's it's


00:28:23.840 --> 00:28:25.510
the best of these globular star clusters


00:28:25.520 --> 00:28:26.870
in the whole sky. It's the biggest and


00:28:26.880 --> 00:28:28.950
best and brightest. It really is very,


00:28:28.960 --> 00:28:31.190
very impressive. Now, low down in the


00:28:31.200 --> 00:28:32.789
eastern sky at mid evening, you got the


00:28:32.799 --> 00:28:34.430
constellation Scorpius above the


00:28:34.440 --> 00:28:37.110
horizon. This, for me, is a true


00:28:37.120 --> 00:28:38.470
indication that the middle of the year


00:28:38.480 --> 00:28:41.350
is upon us because Scorpius is us in the


00:28:41.360 --> 00:28:42.389
southern hemisphere a winter


00:28:42.399 --> 00:28:43.750
constellation. For our friends in the


00:28:43.760 --> 00:28:46.389
north, it's a summer constellation. So,


00:28:46.399 --> 00:28:48.630
as the evening goes on, the full extent


00:28:48.640 --> 00:28:50.389
of Scorpius will come up and and be


00:28:50.399 --> 00:28:52.149
visible. Scorpius is one of the rare


00:28:52.159 --> 00:28:53.590
constellations. It actually looks like


00:28:53.600 --> 00:28:55.590
what it's supposed to be. uh you know


00:28:55.600 --> 00:28:57.029
you've got triang constellation


00:28:57.039 --> 00:28:58.710
triangulum which is a triangle right so


00:28:58.720 --> 00:29:00.549
that's not too hard the southern cross


00:29:00.559 --> 00:29:02.230
does look like a southern cross but


00:29:02.240 --> 00:29:04.070
scorpius really does look like a


00:29:04.080 --> 00:29:05.990
scorpion it traces out the shape of a


00:29:06.000 --> 00:29:08.230
scorpion really really well it's it's


00:29:08.240 --> 00:29:09.269
just one of those things that just


00:29:09.279 --> 00:29:10.389
happen to be in the right part of the


00:29:10.399 --> 00:29:12.149
galaxy to see these stars from this


00:29:12.159 --> 00:29:14.789
point of view and uh yeah it really does


00:29:14.799 --> 00:29:16.310
the constellation right next to it


00:29:16.320 --> 00:29:18.470
famous Sagittarius got no idea what that


00:29:18.480 --> 00:29:19.590
looks like you know it's one of the join


00:29:19.600 --> 00:29:21.190
the dot things but when we do look at


00:29:21.200 --> 00:29:23.510
Sagittarius which was which we you will


00:29:23.520 --> 00:29:26.070
see if you stay past midnight, you'll


00:29:26.080 --> 00:29:27.669
see Sagittarius come up or if you wait


00:29:27.679 --> 00:29:28.950
for a month or two, it'll be in the


00:29:28.960 --> 00:29:30.789
evening sky. When we look towards


00:29:30.799 --> 00:29:32.310
Sagittarius, we are looking into the


00:29:32.320 --> 00:29:34.470
direction of the center of our Milky Way


00:29:34.480 --> 00:29:36.149
galaxy. And this is actually one of the


00:29:36.159 --> 00:29:39.029
main reasons why meteor stargazing is is


00:29:39.039 --> 00:29:40.470
considered so good by amateur


00:29:40.480 --> 00:29:42.470
astronomers because we have all the


00:29:42.480 --> 00:29:44.470
starfields and the deep sky objects of


00:29:44.480 --> 00:29:47.350
the Milky Way central region to enjoy


00:29:47.360 --> 00:29:48.870
because we're looking right into the


00:29:48.880 --> 00:29:50.630
core. There's lots and lots of stuff. If


00:29:50.640 --> 00:29:51.669
you look in the opposite direction,


00:29:51.679 --> 00:29:53.350
you're looking towards the outskirts of


00:29:53.360 --> 00:29:56.470
the galaxy and there's perhaps the left


00:29:56.480 --> 00:29:57.990
sea. So there's a lot of stuff


00:29:58.000 --> 00:30:00.070
concentrated in towards the center of


00:30:00.080 --> 00:30:02.549
our galaxy during the middle of the


00:30:02.559 --> 00:30:04.789
year. And because Sagittarius and it


00:30:04.799 --> 00:30:06.149
sort of surrounding constellations are


00:30:06.159 --> 00:30:07.990
located south of celestial equator, it


00:30:08.000 --> 00:30:09.669
means that those of us who live south of


00:30:09.679 --> 00:30:11.430
the earthly equator get the best view of


00:30:11.440 --> 00:30:13.269
it because from the latitude to where I


00:30:13.279 --> 00:30:15.269
live, it's basically right overhead at


00:30:15.279 --> 00:30:17.430
nighttime. So, you know, you when things


00:30:17.440 --> 00:30:18.549
are right overhead, you're looking


00:30:18.559 --> 00:30:19.909
through the thinnest part of the Earth's


00:30:19.919 --> 00:30:21.430
atmosphere. If things are down on the


00:30:21.440 --> 00:30:23.029
horizon, you're looking through a much


00:30:23.039 --> 00:30:24.789
greater extent of atmosphere, which


00:30:24.799 --> 00:30:26.710
makes the stars appear dimmer and and


00:30:26.720 --> 00:30:28.789
you get twinkling effects and the


00:30:28.799 --> 00:30:31.029
pollution and dust and whatever in the


00:30:31.039 --> 00:30:33.350
air. So, when you can see things up nice


00:30:33.360 --> 00:30:35.590
high, nice up nice and high, that's a


00:30:35.600 --> 00:30:37.190
whole lot better. So, our friends north


00:30:37.200 --> 00:30:38.789
of the equator can certainly see


00:30:38.799 --> 00:30:40.710
Sagittarius and Scorpius as well, but


00:30:40.720 --> 00:30:42.470
for them, it's lower down towards


00:30:42.480 --> 00:30:43.990
they're lower down towards the horizon.


00:30:44.000 --> 00:30:45.909
and it's still good, but nothing like


00:30:45.919 --> 00:30:47.830
being right underneath these particular


00:30:47.840 --> 00:30:49.269
constellations. Now, turning to the


00:30:49.279 --> 00:30:51.350
planets, Jupiter, it's big and bright.


00:30:51.360 --> 00:30:53.830
It's low down near the northwestern


00:30:53.840 --> 00:30:56.630
horizon after sunset. That's as we view


00:30:56.640 --> 00:30:58.149
it from the southern hemisphere during


00:30:58.159 --> 00:31:00.149
May. Now, make sure you take the


00:31:00.159 --> 00:31:02.549
opportunity to see it in the first two


00:31:02.559 --> 00:31:04.149
or three weeks of May because by the end


00:31:04.159 --> 00:31:05.669
of the month, it'll have disappeared


00:31:05.679 --> 00:31:07.909
into the twilight glow down on the


00:31:07.919 --> 00:31:09.669
northwestern horizon there. It's getting


00:31:09.679 --> 00:31:12.310
lower each night. Mars is quite easy to


00:31:12.320 --> 00:31:14.149
see in the northern half of the sky for


00:31:14.159 --> 00:31:15.510
us here in the south or southern half of


00:31:15.520 --> 00:31:17.510
the sky for our friends in the north.


00:31:17.520 --> 00:31:19.269
It's about halfway up from the horizon.


00:31:19.279 --> 00:31:21.990
It's in a fairly bare patch of sky, so


00:31:22.000 --> 00:31:24.549
it's intense ruddy color does make it


00:31:24.559 --> 00:31:26.389
stand out quite easily amongst all the


00:31:26.399 --> 00:31:28.070
stars that are around it. Now, the other


00:31:28.080 --> 00:31:29.669
three bright planets are all morning


00:31:29.679 --> 00:31:31.510
objects at the moment. It's visible out


00:31:31.520 --> 00:31:34.230
to the east before dawn. First up, we


00:31:34.240 --> 00:31:37.669
have Venus. It's extremely bright at the


00:31:37.679 --> 00:31:39.669
moment. You simply cannot miss it or


00:31:39.679 --> 00:31:41.509
mistake it for anything else. Just if


00:31:41.519 --> 00:31:42.950
you're up before dawn, look to the east,


00:31:42.960 --> 00:31:44.470
which is the direction that the sun


00:31:44.480 --> 00:31:46.630
comes up. And before the sun comes up,


00:31:46.640 --> 00:31:48.549
you see this big bright star looking


00:31:48.559 --> 00:31:50.470
thing in the sky. Well, that's Venus.


00:31:50.480 --> 00:31:52.789
That's uh there's nothing else like it.


00:31:52.799 --> 00:31:55.110
Not far from Venus, but quite a bit


00:31:55.120 --> 00:31:57.110
dimmer is another bright thing that


00:31:57.120 --> 00:31:58.590
looks like a star, but it's actually


00:31:58.600 --> 00:32:01.509
Saturn. And Saturn's fairly easy to spot


00:32:01.519 --> 00:32:03.350
because it's, you know, compared to


00:32:03.360 --> 00:32:05.110
other stars or compared to stars, it's


00:32:05.120 --> 00:32:06.710
reasonably bright. It's not bright


00:32:06.720 --> 00:32:08.389
compared to Venus, but it's bright


00:32:08.399 --> 00:32:10.149
enough. And it does have a yellowish


00:32:10.159 --> 00:32:12.870
sort of color to it. Uh about halfway in


00:32:12.880 --> 00:32:14.950
brightness between Saturn and Venus is


00:32:14.960 --> 00:32:16.710
Mercury. The planet Mercury, which is


00:32:16.720 --> 00:32:18.310
the innermost planet. Now, if you want


00:32:18.320 --> 00:32:20.310
to see Mercury, uh yes, you got you got


00:32:20.320 --> 00:32:22.149
to be up before dawn, but you also got


00:32:22.159 --> 00:32:24.630
to get out there and do it now because


00:32:24.640 --> 00:32:26.789
as the month goes on, you'll see Venus


00:32:26.799 --> 00:32:29.430
and Saturn still up fairly high, moving


00:32:29.440 --> 00:32:30.870
further apart from each other, but


00:32:30.880 --> 00:32:32.310
Mercury is going to start dropping down


00:32:32.320 --> 00:32:34.070
toward the horizon for night after


00:32:34.080 --> 00:32:35.909
night. By the end of the third week of


00:32:35.919 --> 00:32:39.190
May, it'll be lost in the glare of the


00:32:39.200 --> 00:32:42.470
uh dawn glory just before sunrise. So


00:32:42.480 --> 00:32:43.909
yeah, if you want to spot Mercury, if


00:32:43.919 --> 00:32:45.430
you've never seen it before, got to be


00:32:45.440 --> 00:32:47.350
up before dawn and got to do it in the


00:32:47.360 --> 00:32:49.029
next few weeks. And let's do Stewart is


00:32:49.039 --> 00:32:50.950
the sky formation. That's science writer


00:32:50.960 --> 00:32:54.980
Jonathan Nelly and this is Spaceime.


00:32:54.990 --> 00:33:08.870
[Music]


00:33:08.880 --> 00:33:11.669
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