- published: 18 Apr 2019
- views: 19167
Create your page here
Halo-
Halo- is a Greek prefix meaning "salt." In biology, it is often used to indicate halotolerance and is a portion of many words:
See also
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Halo-
Halo (Current 93 album)
Halo is a live album, released in 2004, by Current 93. The front cover is a drawing by the same David Tibet which reproduces the cover of a Moody Blues album of 1971 Every Good Boy Deserves Favour.
Track listing
References
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Halo_(Current_93_album)
Halo (UK band)
Halo are a rock band from Bristol, England, who formed in 1999 and disbanded in 2004. In 2002, they released one album, and had three singles in the UK Singles Chart. They reformed in 2011 and are currently recording their second album.
History
The band’s journey began in 1999 when brothers Graeme and Iain Moncrieff joined forces with Jim Davey and then Stevie Yeomans. They developed a unique sound consisting of raw energy, soaring guitars, an unswerving rhythm section, epic songs and rich three-part vocal harmony.
Halo quickly gained a reputation for their electrifying live shows and soon found themselves on the radar of publishing giants Windswept Pacific, who snapped them up immediately after watching the band perform at The Astoria, London. Shortly afterwards Sony’s S2 label became favourites to sign them and the band promptly put pen to paper with Muff Winwood, head of Sony Europe, to sign a six album deal.
Halo’s first release, the ‘Still Here’ EP, was recorded in London and given away free to their rapidly expanding fan base with rave reviews. Kerrang urged readers not to ‘look this gift stallion in the mouth’ and to join Halo’s mailing list pronto.
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Halo_(UK_band)
Podcasts:
Halo
ALBUMS
- Heaven Calling released: 1991
- Halo released: 1989
Halo
ALBUMS
- V živo released: 2003
- Kaj je novega? released: 1999
- Anita ni nikoli ... released: 1997
Halo
ALBUMS
- Mansa Musa released: 2014
Halo
ALBUMS
- Lunatic Ride released: 2002
Halo
ALBUMS
- Seventy Dubstep Electronic Essentials released: 2012
헤일로
ALBUMS
- Hello HALO released: 2014
- 38℃ released: 2014
Halo
ALBUMS
- Live 06:06:01 released: 2004
- Degree Zero: Point of Implosion released: 2004
- Body of Light released: 2003
- Massive Corporate Disease released: 1999
- Guattari: From the West Flows Grey Ash and Pestilence released: 1999
- Subliminal Transmissions released: 1998
HaLo
Halo
ALBUMS
- Fabric 07: Hipp-E & Halo released: 2002
- Muzik Box released: 1999
Fabric 07: Hipp-E & Halo
Released 2002- Slow Swing
- 3 in tha Mornin' (Swag's version dub)
- Metroride (Ken & Sams Racketride)
- I'm Satisfied
- Freakinought
- Time (Doza's Lawnchair Generals mix)
- Mumbo Jumbo (Kitchen Dwellers)
- Rugburns (original mix)
- And I Know
- Midnight (dub mix)
- Long Deep Decay
- When I Fell in Love (Charles Webster dub mix)
- Lakeshore Dr.
- Body Flowers (Fluid System mix)
Ha-Lo
ALBUMS
- The Sound of Eukatech 5 released: 2001
- Nocturnal released: 2000
- Rapid Descent released: 1999
- DJ Excursions, Volume 2 - Diversatility released: 1997
- Mazzo Mixup - Sex Love & Motion 1 + 2 released: 1997
- In the Mix, Volume 2: The Colours of Sound released: 1996
H.A.L.O.
ALBUMS
- Immanent released: 1994
Halo
ALBUMS
-
Classroom Aid - The Galactic Halo
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf In this segment of our “How far away is it” video book, we cover the structure of the Milky Way galaxy. We start with a high-level description of the three main components: the galactic center with its black hole, the galactic disk with its spiral arms, and the galactic halo stretching far out in all directions using the European Space Agency spacecraft Gaia’s findings. We also show how full images of the Milky Way can be created from within the galaxy. Using the full power of the Hubble, Spitzer, and Chandra space telescopes, we take a deep dive into the center of our galaxy with its central bulge. We detail the evidence for the existence of a supermassive black hole, Sagittarius A*, at the very center ...
published: 18 Apr 2019 -
Teach Astronomy - Galactic Halo
http://www.teachastronomy.com/ The halo of the Milky Way galaxy is traced by the globular clusters and by individual stars that are dim and which contain a far lower metal abundance than the Sun or stars in the solar neighborhood. The distribution of globular clusters on the plane of the sky gives a clue both to the shape of the galaxy and to the Sun's position within that distribution. For example, if we were at the center of a spherical cloud of globular clusters, we would count equal numbers in each direction in the sky, but if we were offset from the center, we would count more clusters in the direction towards the center. This simple technique was used by Harlow Shapley in the 1930s to show that the Milky Way was indeed spherical in the shape of its halo and that the Sun was not at...
published: 23 Jul 2010 -
Galactic Disk Structure | Milky way rotation curves | Galactic Halo
Join this channel to get access to perks: https://www.youtube.com/channel/UCdZk5f22y0vCq5ePh4h3gAA/join Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust). The stellar population of galactic discs tends to exhibit very little random motion with most of its stars undergoing nearly circular orbits about the galactic center. Here we cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look ...
published: 25 Feb 2021 -
Most Distant Halo Stars in Milky Way Are Halfway to Andromeda Galaxy
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath More cool designs are on Amazon: https://amzn.to/3wDGy2i Alternatively, PayPal donations can be sent here: http://paypal.me/whatdamath Hello and welcome! My name is Anton and in this video, we will talk about a discovery of very distant Milky Way stars that are part of the outer halo Links: https://aas.org/meetings/aas241 https://news.ucsc.edu/2023/01/milky-way-halo.html https://en.wikipedia.org/wiki/RR_Lyrae_variable Major Milky Way discoveries: https://youtu.be/IwvZavzQPgc #milkyway #rrlyrae #halo 0:00 Intro to Halo Stars 1:00 Milky Way discoveries 2:20 Variable stars and how they work 3:25 RR Lyrae stars 5:45 New study and discoveries Support this channel on Patreon to help me make this a full time job: https://ww...
published: 17 Jan 2023 -
The Mysteries Of The Galactic Halo!
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-minute video, we explore the mysteries of this ancient and enigmatic part of our universe. We delve into the origin and nature of the galactic halo, including its unique properties and the mysteries it holds. Through stunning visuals and expert insights, we investigate the possibility of dark matter and other unknown elements that exist within the halo. Ultimately, the video portrays the galactic halo as a place of immense curiosity and potential discovery, where we may find answers to some of the most fundamental questions of our existence. Join us on this journey to explore the mysteries of the galactic halo and unlock the secrets of our universe.
published: 23 Apr 2023 -
Milky Way Halo Is 1000 Times Hotter Than Sun's Surface
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6 Or get a shirt: https://teespring.com/stores/whatdamath Hello and welcome! My name is Anton and in this video, we will talk about new research that discovered that the halo of the milky way galaxy is ridiculously hot. Originally presented here: https://aas.org/meetings/aas236 Support this channel on Patreon to help me make this a full time job: https://www.patreon.com/whatdamath Space Engine is available for free here: http://spaceengine.org Enjoy and please subscribe. Twitter: https://twitter.com/WhatDaMath Facebook: https://www.facebook.com/whatdamath Twitch: http://www.twitch.tv/whatdamath Bitcoins to spare? Donate them here to help this channel grow! 1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu Alternatively, PayPal donations c...
published: 13 Jun 2020 -
Probing a galactic halo with Hubble
This animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble's Cosmic Origins Spectrograph (COS) to probe faint galactic envelopes by exploiting even more distant objects — quasars, the intensely luminous centres of distant galaxies powered by huge black holes. As the light from the distant quasar passes through the galaxy's halo, the gas absorbs certain frequencies -- making it possible to study the region around the galaxy in detail. This new research utilised Hubble's COS to peer through the very thin outskirts of galactic halos, much further out than shown in this representation, to explore galactic gas at distances of up to twenty times greater than the visible size of the galaxy itself. More information and download-option...
published: 25 Apr 2013 -
Halo 4 OST - To Galaxy
Tenth track of the Halo 4 Original Soundtrack
published: 10 Nov 2012 -
To Galaxy
Provided to YouTube by Republic of Music To Galaxy · Halo · Neil Davidge Halo 4 ℗ Microsoft Studios Released on: 2012-10-19 Auto-generated by YouTube.
published: 14 Apr 2023 -
Andromeda Has A Supermassive Halo
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive halo of gas surrounding the Andromeda galaxy. The halo is so big it's interacting with the Milky Way's halo. Source: https://iopscience.iop.org/article/10.3847/1538-4357/aba49c Support us on Patreon and help Cosmoknowledge become the number one destination for science: https://www.patreon.com/cosmoknowledge SUBSCRIBE ► https://goo.gl/PLLFPz ---- Website ► https://cosmoknowledge.com/ TikTok ► https://www.tiktok.com/@cosmoknowledge Instagram ► https://www.instagram.com/itscosmoknowledge Facebook ► https://facebook.com/cosmoknowledgee Edited by: Ardit Bicaj Narrated by: Russell Archey https://www.ravonmedia.com/ Graphics & Credits: Space Engine Universe Sandbox 2 NASA, ESA, J. DePasquale and E. Whe...
published: 12 Sep 2020
developed with YouTube
3:18
Classroom Aid - The Galactic Halo
- Order: Reorder
- Duration: 3:18
- Uploaded Date: 18 Apr 2019
- views: 19167
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf
In this segment of our “How far away is it” video book, we cover the struct...
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf
In this segment of our “How far away is it” video book, we cover the structure of the Milky Way galaxy.
We start with a high-level description of the three main components: the galactic center with its black hole, the galactic disk with its spiral arms, and the galactic halo stretching far out in all directions using the European Space Agency spacecraft Gaia’s findings. We also show how full images of the Milky Way can be created from within the galaxy.
Using the full power of the Hubble, Spitzer, and Chandra space telescopes, we take a deep dive into the center of our galaxy with its central bulge. We detail the evidence for the existence of a supermassive black hole, Sagittarius A*, at the very center of the galaxy’s core. We cover and illustrate the work done by the UCLA Galactic Centre Group in conjunction with the new Keck observatory on top of the Mauna Kea volcano in Hawaii, and the Max Plank Institute for Extraterrestrial Physics in Germany and more recently and the European Southern Observatory with its array of Very Large Telescopes in Chile. This includes a look at how close the star S2 approached Sgr A* and what that black hole might look like. In addition, we cover stellar interferometry with ducks on a pond to see how these measurements were done.
Next, we go a level deeper into the nature of a Black Hole singularity. We cover the Schwarzschild radius, event horizon, accretion disk, gravitational lensing, and gamma-ray jets. We then actually build Sgr A*. In addition to the supermassive black hole, we take a look at a solar mass black hole.
We then cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
https://wn.com/Classroom_Aid_The_Galactic_Halo
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf
In this segment of our “How far away is it” video book, we cover the structure of the Milky Way galaxy.
We start with a high-level description of the three main components: the galactic center with its black hole, the galactic disk with its spiral arms, and the galactic halo stretching far out in all directions using the European Space Agency spacecraft Gaia’s findings. We also show how full images of the Milky Way can be created from within the galaxy.
Using the full power of the Hubble, Spitzer, and Chandra space telescopes, we take a deep dive into the center of our galaxy with its central bulge. We detail the evidence for the existence of a supermassive black hole, Sagittarius A*, at the very center of the galaxy’s core. We cover and illustrate the work done by the UCLA Galactic Centre Group in conjunction with the new Keck observatory on top of the Mauna Kea volcano in Hawaii, and the Max Plank Institute for Extraterrestrial Physics in Germany and more recently and the European Southern Observatory with its array of Very Large Telescopes in Chile. This includes a look at how close the star S2 approached Sgr A* and what that black hole might look like. In addition, we cover stellar interferometry with ducks on a pond to see how these measurements were done.
Next, we go a level deeper into the nature of a Black Hole singularity. We cover the Schwarzschild radius, event horizon, accretion disk, gravitational lensing, and gamma-ray jets. We then actually build Sgr A*. In addition to the supermassive black hole, we take a look at a solar mass black hole.
We then cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
1:04
Teach Astronomy - Galactic Halo
- Order: Reorder
- Duration: 1:04
- Uploaded Date: 23 Jul 2010
- views: 764
http://www.teachastronomy.com/
The halo of the Milky Way galaxy is traced by the globular clusters and by individual stars that are dim and which contain a far ...
http://www.teachastronomy.com/
The halo of the Milky Way galaxy is traced by the globular clusters and by individual stars that are dim and which contain a far lower metal abundance than the Sun or stars in the solar neighborhood. The distribution of globular clusters on the plane of the sky gives a clue both to the shape of the galaxy and to the Sun's position within that distribution. For example, if we were at the center of a spherical cloud of globular clusters, we would count equal numbers in each direction in the sky, but if we were offset from the center, we would count more clusters in the direction towards the center. This simple technique was used by Harlow Shapley in the 1930s to show that the Milky Way was indeed spherical in the shape of its halo and that the Sun was not at the center of the distribution but was offset by eight or nine thousand parsecs from the center which was in the direction of the constellation Sagittarius.
https://wn.com/Teach_Astronomy_Galactic_Halo
http://www.teachastronomy.com/
The halo of the Milky Way galaxy is traced by the globular clusters and by individual stars that are dim and which contain a far lower metal abundance than the Sun or stars in the solar neighborhood. The distribution of globular clusters on the plane of the sky gives a clue both to the shape of the galaxy and to the Sun's position within that distribution. For example, if we were at the center of a spherical cloud of globular clusters, we would count equal numbers in each direction in the sky, but if we were offset from the center, we would count more clusters in the direction towards the center. This simple technique was used by Harlow Shapley in the 1930s to show that the Milky Way was indeed spherical in the shape of its halo and that the Sun was not at the center of the distribution but was offset by eight or nine thousand parsecs from the center which was in the direction of the constellation Sagittarius.
- published: 23 Jul 2010
- views: 764
13:08
Galactic Disk Structure | Milky way rotation curves | Galactic Halo
- Order: Reorder
- Duration: 13:08
- Uploaded Date: 25 Feb 2021
- views: 3112
Join this channel to get access to perks:
https://www.youtube.com/channel/UCdZk5f22y0vCq5ePh4h3gAA/join
Galactic discs consist of a stellar component (composed...
Join this channel to get access to perks:
https://www.youtube.com/channel/UCdZk5f22y0vCq5ePh4h3gAA/join
Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust). The stellar population of galactic discs tends to exhibit very little random motion with most of its stars undergoing nearly circular orbits about the galactic center.
Here we cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
#GalacticDiskStructure
#MilkyWay
#GalacticHalo
https://wn.com/Galactic_Disk_Structure_|_Milky_Way_Rotation_Curves_|_Galactic_Halo
Join this channel to get access to perks:
https://www.youtube.com/channel/UCdZk5f22y0vCq5ePh4h3gAA/join
Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust). The stellar population of galactic discs tends to exhibit very little random motion with most of its stars undergoing nearly circular orbits about the galactic center.
Here we cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
#GalacticDiskStructure
#MilkyWay
#GalacticHalo
- published: 25 Feb 2021
- views: 3112
10:42
Most Distant Halo Stars in Milky Way Are Halfway to Andromeda Galaxy
- Order: Reorder
- Duration: 10:42
- Uploaded Date: 17 Jan 2023
- views: 94048
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath
More cool designs are on Amazon: https://amzn.to/3wDGy2i
Alternatively, PayPal donations can...
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath
More cool designs are on Amazon: https://amzn.to/3wDGy2i
Alternatively, PayPal donations can be sent here: http://paypal.me/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about a discovery of very distant Milky Way stars that are part of the outer halo
Links:
https://aas.org/meetings/aas241
https://news.ucsc.edu/2023/01/milky-way-halo.html
https://en.wikipedia.org/wiki/RR_Lyrae_variable
Major Milky Way discoveries: https://youtu.be/IwvZavzQPgc
#milkyway #rrlyrae #halo
0:00 Intro to Halo Stars
1:00 Milky Way discoveries
2:20 Variable stars and how they work
3:25 RR Lyrae stars
5:45 New study and discoveries
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Bitcoin/Ethereum to spare? Donate them here to help this channel grow!
bc1qnkl3nk0zt7w0xzrgur9pnkcduj7a3xxllcn7d4
or ETH: 0x60f088B10b03115405d313f964BeA93eF0Bd3DbF
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
The hardware used to record these videos:
New Camera: https://amzn.to/34DUUlv
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Special thanks also goes to all the wonderful supporters of the channel through YouTube Memberships
Images/Videos:
NASA, ESA, and A. Feild (STScI)
Antonio Ciccolella CC BY-SA 4.0 https://en.wikipedia.org/wiki/Local_Group#/media/File:Local_Group_and_nearest_galaxies.jpg
RJHall CC BY-SA 3.0 https://en.wikipedia.org/wiki/RR_Lyrae_variable#/media/File:Rr_lyrae_ltcrv_en.svg
Chris Mihos (Case Western Reserve University)/ESO -CC BY 4.0 https://en.wikipedia.org/wiki/Virgo_Cluster#/media/File:ESO-M87.jpg
ESO/VVV Survey/D. Minniti - https://www.eso.org/public/images/eso1636a/ CC BY 4.0
Licenses used:
https://creativecommons.org/licenses/by/4.0/
https://creativecommons.org/licenses/by-sa/4.0/
https://creativecommons.org/licenses/by/3.0/
https://creativecommons.org/licenses/by-sa/3.0/
https://creativecommons.org/licenses/by/2.5/
https://creativecommons.org/licenses/by-sa/2.5/
https://creativecommons.org/licenses/by/2.0/
https://creativecommons.org/licenses/by-sa/2.0/
https://wn.com/Most_Distant_Halo_Stars_In_Milky_Way_Are_Halfway_To_Andromeda_Galaxy
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath
More cool designs are on Amazon: https://amzn.to/3wDGy2i
Alternatively, PayPal donations can be sent here: http://paypal.me/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about a discovery of very distant Milky Way stars that are part of the outer halo
Links:
https://aas.org/meetings/aas241
https://news.ucsc.edu/2023/01/milky-way-halo.html
https://en.wikipedia.org/wiki/RR_Lyrae_variable
Major Milky Way discoveries: https://youtu.be/IwvZavzQPgc
#milkyway #rrlyrae #halo
0:00 Intro to Halo Stars
1:00 Milky Way discoveries
2:20 Variable stars and how they work
3:25 RR Lyrae stars
5:45 New study and discoveries
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Bitcoin/Ethereum to spare? Donate them here to help this channel grow!
bc1qnkl3nk0zt7w0xzrgur9pnkcduj7a3xxllcn7d4
or ETH: 0x60f088B10b03115405d313f964BeA93eF0Bd3DbF
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
The hardware used to record these videos:
New Camera: https://amzn.to/34DUUlv
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Special thanks also goes to all the wonderful supporters of the channel through YouTube Memberships
Images/Videos:
NASA, ESA, and A. Feild (STScI)
Antonio Ciccolella CC BY-SA 4.0 https://en.wikipedia.org/wiki/Local_Group#/media/File:Local_Group_and_nearest_galaxies.jpg
RJHall CC BY-SA 3.0 https://en.wikipedia.org/wiki/RR_Lyrae_variable#/media/File:Rr_lyrae_ltcrv_en.svg
Chris Mihos (Case Western Reserve University)/ESO -CC BY 4.0 https://en.wikipedia.org/wiki/Virgo_Cluster#/media/File:ESO-M87.jpg
ESO/VVV Survey/D. Minniti - https://www.eso.org/public/images/eso1636a/ CC BY 4.0
Licenses used:
https://creativecommons.org/licenses/by/4.0/
https://creativecommons.org/licenses/by-sa/4.0/
https://creativecommons.org/licenses/by/3.0/
https://creativecommons.org/licenses/by-sa/3.0/
https://creativecommons.org/licenses/by/2.5/
https://creativecommons.org/licenses/by-sa/2.5/
https://creativecommons.org/licenses/by/2.0/
https://creativecommons.org/licenses/by-sa/2.0/
- published: 17 Jan 2023
- views: 94048
0:56
The Mysteries Of The Galactic Halo!
- Order: Reorder
- Duration: 0:56
- Uploaded Date: 23 Apr 2023
- views: 189
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-minute video, we explore the mysteries of this ancient and enigmatic part...
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-minute video, we explore the mysteries of this ancient and enigmatic part of our universe. We delve into the origin and nature of the galactic halo, including its unique properties and the mysteries it holds. Through stunning visuals and expert insights, we investigate the possibility of dark matter and other unknown elements that exist within the halo. Ultimately, the video portrays the galactic halo as a place of immense curiosity and potential discovery, where we may find answers to some of the most fundamental questions of our existence. Join us on this journey to explore the mysteries of the galactic halo and unlock the secrets of our universe.
https://wn.com/The_Mysteries_Of_The_Galactic_Halo
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-minute video, we explore the mysteries of this ancient and enigmatic part of our universe. We delve into the origin and nature of the galactic halo, including its unique properties and the mysteries it holds. Through stunning visuals and expert insights, we investigate the possibility of dark matter and other unknown elements that exist within the halo. Ultimately, the video portrays the galactic halo as a place of immense curiosity and potential discovery, where we may find answers to some of the most fundamental questions of our existence. Join us on this journey to explore the mysteries of the galactic halo and unlock the secrets of our universe.
- published: 23 Apr 2023
- views: 189
9:13
Milky Way Halo Is 1000 Times Hotter Than Sun's Surface
- Order: Reorder
- Duration: 9:13
- Uploaded Date: 13 Jun 2020
- views: 83490
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6
Or get a shirt: https://teespring.com/stores/whatdamath
Hello and welcome! My name is Anton and in...
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6
Or get a shirt: https://teespring.com/stores/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about new research that discovered that the halo of the milky way galaxy is ridiculously hot.
Originally presented here: https://aas.org/meetings/aas236
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
Bitcoins to spare? Donate them here to help this channel grow!
1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu
Alternatively, PayPal donations can be sent here: https://www.paypal.com/cgi-bin/webscr?cmd=_s-xclick&hosted_button_id=DNKM9SDWU3B3Q&source=url
The hardware used to record these videos:
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Specifically, great thanks to the following members:
Morrison Waud
Vlad Manshin
Mark Teranishi
TheHuntress
Ralph Spataro
Albert B. Cannon
Lilith Dawn
Greg Lambros
adam lee
Gabriel Seiffert
Henry Spadoni
J Carter
Jer
Silver surfer
Konrad Kummli
Nick Dolgy
UnexpectedBooks.com
Mario Rahmani
George Williams
Shinne
Jakub Glos
Johann Goergen
Jake Salo
LS Greger
Lyndon Riley
Lauren Smith
Michael Tiganila
Russell Sears
Vinod sethi
Dave Blair
Robert Wyssbrod
Randal Masutani
Michael Mitsuda
Assaf Dar Sagol
Liam Moss
Timothy Welter MD
Barnard Rabenold
Gordon Cooper
Tracy Burgess
Douglas Burns
Jayjay Volz
Anataine Deva
Kai Raphahn
Sander Stols
Bodo Graßmann
Daniel Charles Smith
Daniel G.
Eugene Sandulenko
gary steelman
Max McNally
Michael Koebel
Sergio Ruelas
Steven Aiello
Victor Julian Castillo
xyndicate
Honey Suzanne Lyons
Olegas Budnik
Dale Andrew Darling
Niji
Peter Hamrak
Matthew Lazear
Alexander Afanasyev
Anton Newman
Anton Reed
https://wn.com/Milky_Way_Halo_Is_1000_Times_Hotter_Than_Sun's_Surface
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6
Or get a shirt: https://teespring.com/stores/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about new research that discovered that the halo of the milky way galaxy is ridiculously hot.
Originally presented here: https://aas.org/meetings/aas236
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
Bitcoins to spare? Donate them here to help this channel grow!
1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu
Alternatively, PayPal donations can be sent here: https://www.paypal.com/cgi-bin/webscr?cmd=_s-xclick&hosted_button_id=DNKM9SDWU3B3Q&source=url
The hardware used to record these videos:
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Specifically, great thanks to the following members:
Morrison Waud
Vlad Manshin
Mark Teranishi
TheHuntress
Ralph Spataro
Albert B. Cannon
Lilith Dawn
Greg Lambros
adam lee
Gabriel Seiffert
Henry Spadoni
J Carter
Jer
Silver surfer
Konrad Kummli
Nick Dolgy
UnexpectedBooks.com
Mario Rahmani
George Williams
Shinne
Jakub Glos
Johann Goergen
Jake Salo
LS Greger
Lyndon Riley
Lauren Smith
Michael Tiganila
Russell Sears
Vinod sethi
Dave Blair
Robert Wyssbrod
Randal Masutani
Michael Mitsuda
Assaf Dar Sagol
Liam Moss
Timothy Welter MD
Barnard Rabenold
Gordon Cooper
Tracy Burgess
Douglas Burns
Jayjay Volz
Anataine Deva
Kai Raphahn
Sander Stols
Bodo Graßmann
Daniel Charles Smith
Daniel G.
Eugene Sandulenko
gary steelman
Max McNally
Michael Koebel
Sergio Ruelas
Steven Aiello
Victor Julian Castillo
xyndicate
Honey Suzanne Lyons
Olegas Budnik
Dale Andrew Darling
Niji
Peter Hamrak
Matthew Lazear
Alexander Afanasyev
Anton Newman
Anton Reed
- published: 13 Jun 2020
- views: 83490
0:47
Probing a galactic halo with Hubble
- Order: Reorder
- Duration: 0:47
- Uploaded Date: 25 Apr 2013
- views: 1586
This animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble's Cosmic Origins Spectrograph (COS) to p...
This animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble's Cosmic Origins Spectrograph (COS) to probe faint galactic envelopes by exploiting even more distant objects — quasars, the intensely luminous centres of distant galaxies powered by huge black holes.
As the light from the distant quasar passes through the galaxy's halo, the gas absorbs certain frequencies -- making it possible to study the region around the galaxy in detail.
This new research utilised Hubble's COS to peer through the very thin outskirts of galactic halos, much further out than shown in this representation, to explore galactic gas at distances of up to twenty times greater than the visible size of the galaxy itself.
More information and download-options:
http://www.spacetelescope.org/videos/heic1308a/
Credit:
ESA, NASA, L. Calçada
https://wn.com/Probing_A_Galactic_Halo_With_Hubble
This animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble's Cosmic Origins Spectrograph (COS) to probe faint galactic envelopes by exploiting even more distant objects — quasars, the intensely luminous centres of distant galaxies powered by huge black holes.
As the light from the distant quasar passes through the galaxy's halo, the gas absorbs certain frequencies -- making it possible to study the region around the galaxy in detail.
This new research utilised Hubble's COS to peer through the very thin outskirts of galactic halos, much further out than shown in this representation, to explore galactic gas at distances of up to twenty times greater than the visible size of the galaxy itself.
More information and download-options:
http://www.spacetelescope.org/videos/heic1308a/
Credit:
ESA, NASA, L. Calçada
- published: 25 Apr 2013
- views: 1586
4:58
Halo 4 OST - To Galaxy
- Order: Reorder
- Duration: 4:58
- Uploaded Date: 10 Nov 2012
- views: 509171
Tenth track of the Halo 4 Original Soundtrack
Tenth track of the Halo 4 Original Soundtrack
https://wn.com/Halo_4_Ost_To_Galaxy
Tenth track of the Halo 4 Original Soundtrack
- published: 10 Nov 2012
- views: 509171
5:03
To Galaxy
- Order: Reorder
- Duration: 5:03
- Uploaded Date: 14 Apr 2023
- views: 14581
Provided to YouTube by Republic of Music
To Galaxy · Halo · Neil Davidge
Halo 4
℗ Microsoft Studios
Released on: 2012-10-19
Auto-generated by YouTube.
Provided to YouTube by Republic of Music
To Galaxy · Halo · Neil Davidge
Halo 4
℗ Microsoft Studios
Released on: 2012-10-19
Auto-generated by YouTube.
https://wn.com/To_Galaxy
Provided to YouTube by Republic of Music
To Galaxy · Halo · Neil Davidge
Halo 4
℗ Microsoft Studios
Released on: 2012-10-19
Auto-generated by YouTube.
- published: 14 Apr 2023
- views: 14581
3:36
Andromeda Has A Supermassive Halo
- Order: Reorder
- Duration: 3:36
- Uploaded Date: 12 Sep 2020
- views: 2364
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive halo of gas surrounding the Andromeda galaxy. The halo is so big it's...
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive halo of gas surrounding the Andromeda galaxy. The halo is so big it's interacting with the Milky Way's halo.
Source: https://iopscience.iop.org/article/10.3847/1538-4357/aba49c
Support us on Patreon and help Cosmoknowledge become the number one destination for science: https://www.patreon.com/cosmoknowledge
SUBSCRIBE ► https://goo.gl/PLLFPz
----
Website ► https://cosmoknowledge.com/
TikTok ► https://www.tiktok.com/@cosmoknowledge
Instagram ► https://www.instagram.com/itscosmoknowledge
Facebook ► https://facebook.com/cosmoknowledgee
Edited by:
Ardit Bicaj
Narrated by:
Russell Archey
https://www.ravonmedia.com/
Graphics & Credits:
Space Engine
Universe Sandbox 2
NASA, ESA, J. DePasquale and E. Wheatley (STScI), and Z. Levay
Music:
Close Encounter - Wendel Scherer
Thank you to our Patrons:
DonPig
-
Cosmoknowledge brings news from space.
We love you, explorers!
https://wn.com/Andromeda_Has_A_Supermassive_Halo
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive halo of gas surrounding the Andromeda galaxy. The halo is so big it's interacting with the Milky Way's halo.
Source: https://iopscience.iop.org/article/10.3847/1538-4357/aba49c
Support us on Patreon and help Cosmoknowledge become the number one destination for science: https://www.patreon.com/cosmoknowledge
SUBSCRIBE ► https://goo.gl/PLLFPz
----
Website ► https://cosmoknowledge.com/
TikTok ► https://www.tiktok.com/@cosmoknowledge
Instagram ► https://www.instagram.com/itscosmoknowledge
Facebook ► https://facebook.com/cosmoknowledgee
Edited by:
Ardit Bicaj
Narrated by:
Russell Archey
https://www.ravonmedia.com/
Graphics & Credits:
Space Engine
Universe Sandbox 2
NASA, ESA, J. DePasquale and E. Wheatley (STScI), and Z. Levay
Music:
Close Encounter - Wendel Scherer
Thank you to our Patrons:
DonPig
-
Cosmoknowledge brings news from space.
We love you, explorers!
- published: 12 Sep 2020
- views: 2364
3:18
Classroom Aid - The Galactic Halo
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf
In th...
published: 18 Apr 2019
Classroom Aid - The Galactic Halo
Classroom Aid - The Galactic Halo
- Report rights infringement
- published: 18 Apr 2019
- views: 19167
http://howfarawayisit.com/wp-content/uploads/2019/04/The-Milky-Way-2019-edition.pdf
In this segment of our “How far away is it” video book, we cover the structure of the Milky Way galaxy.
We start with a high-level description of the three main components: the galactic center with its black hole, the galactic disk with its spiral arms, and the galactic halo stretching far out in all directions using the European Space Agency spacecraft Gaia’s findings. We also show how full images of the Milky Way can be created from within the galaxy.
Using the full power of the Hubble, Spitzer, and Chandra space telescopes, we take a deep dive into the center of our galaxy with its central bulge. We detail the evidence for the existence of a supermassive black hole, Sagittarius A*, at the very center of the galaxy’s core. We cover and illustrate the work done by the UCLA Galactic Centre Group in conjunction with the new Keck observatory on top of the Mauna Kea volcano in Hawaii, and the Max Plank Institute for Extraterrestrial Physics in Germany and more recently and the European Southern Observatory with its array of Very Large Telescopes in Chile. This includes a look at how close the star S2 approached Sgr A* and what that black hole might look like. In addition, we cover stellar interferometry with ducks on a pond to see how these measurements were done.
Next, we go a level deeper into the nature of a Black Hole singularity. We cover the Schwarzschild radius, event horizon, accretion disk, gravitational lensing, and gamma-ray jets. We then actually build Sgr A*. In addition to the supermassive black hole, we take a look at a solar mass black hole.
We then cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
1:04
Teach Astronomy - Galactic Halo
http://www.teachastronomy.com/
The halo of the Milky Way galaxy is traced by the globular ...
published: 23 Jul 2010
Teach Astronomy - Galactic Halo
Teach Astronomy - Galactic Halo
- Report rights infringement
- published: 23 Jul 2010
- views: 764
http://www.teachastronomy.com/
The halo of the Milky Way galaxy is traced by the globular clusters and by individual stars that are dim and which contain a far lower metal abundance than the Sun or stars in the solar neighborhood. The distribution of globular clusters on the plane of the sky gives a clue both to the shape of the galaxy and to the Sun's position within that distribution. For example, if we were at the center of a spherical cloud of globular clusters, we would count equal numbers in each direction in the sky, but if we were offset from the center, we would count more clusters in the direction towards the center. This simple technique was used by Harlow Shapley in the 1930s to show that the Milky Way was indeed spherical in the shape of its halo and that the Sun was not at the center of the distribution but was offset by eight or nine thousand parsecs from the center which was in the direction of the constellation Sagittarius.
13:08
Galactic Disk Structure | Milky way rotation curves | Galactic Halo
Join this channel to get access to perks:
https://www.youtube.com/channel/UCdZk5f22y0vCq5e...
published: 25 Feb 2021
Galactic Disk Structure | Milky way rotation curves | Galactic Halo
Galactic Disk Structure | Milky way rotation curves | Galactic Halo
- Report rights infringement
- published: 25 Feb 2021
- views: 3112
Join this channel to get access to perks:
https://www.youtube.com/channel/UCdZk5f22y0vCq5ePh4h3gAA/join
Galactic discs consist of a stellar component (composed of most of the galaxy's stars) and a gaseous component (mostly composed of cool gas and dust). The stellar population of galactic discs tends to exhibit very little random motion with most of its stars undergoing nearly circular orbits about the galactic center.
Here we cover the structure of the galactic disk including: the bar core, the two 3 Parsec arms, Scutum-Centaurus, Perseus, Sagittarius with its Orion Spur, Norma and the Outer Arm. We review the locations of various celestial objects we’ve seen in previous Milky Way segments, to show how close to us they are. We also cover the disk’s rotation and the Sun’s orbit. We look at our solar system’s Ecliptic Plane with respect to the galactic plane. And we cover the galaxy’s dust clouds and how we see them with radio astronomy. We also cover the galaxy’s rotation curve and its connection with dark matter.
Next, we cover the galactic halo. We start with Shapley’s globular cluster map that first showed that we were not at the center of the galaxy. We cover the size of the halo, the inner and outer halos orbital motion, and the newly discovered galaxy within our galaxy called Gaia-Enceladus. We end with recent discoveries of massive amounts of Hydrogen in the halo and this findings impact on the Dark Matter debate. And we end with a calculation of the entire Milky Way’s mass.
We end our galaxy coverage by illustrating how far one would have to go to take a picture that would include what we see in our illustrations. We conclude the chapter with another look at the distance ladder that took us across the galaxy.
#GalacticDiskStructure
#MilkyWay
#GalacticHalo
10:42
Most Distant Halo Stars in Milky Way Are Halfway to Andromeda Galaxy
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath
More cool designs are ...
published: 17 Jan 2023
Most Distant Halo Stars in Milky Way Are Halfway to Andromeda Galaxy
Most Distant Halo Stars in Milky Way Are Halfway to Andromeda Galaxy
- Report rights infringement
- published: 17 Jan 2023
- views: 94048
Get a Wonderful Person Tee: https://teespring.com/stores/whatdamath
More cool designs are on Amazon: https://amzn.to/3wDGy2i
Alternatively, PayPal donations can be sent here: http://paypal.me/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about a discovery of very distant Milky Way stars that are part of the outer halo
Links:
https://aas.org/meetings/aas241
https://news.ucsc.edu/2023/01/milky-way-halo.html
https://en.wikipedia.org/wiki/RR_Lyrae_variable
Major Milky Way discoveries: https://youtu.be/IwvZavzQPgc
#milkyway #rrlyrae #halo
0:00 Intro to Halo Stars
1:00 Milky Way discoveries
2:20 Variable stars and how they work
3:25 RR Lyrae stars
5:45 New study and discoveries
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Bitcoin/Ethereum to spare? Donate them here to help this channel grow!
bc1qnkl3nk0zt7w0xzrgur9pnkcduj7a3xxllcn7d4
or ETH: 0x60f088B10b03115405d313f964BeA93eF0Bd3DbF
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
The hardware used to record these videos:
New Camera: https://amzn.to/34DUUlv
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Special thanks also goes to all the wonderful supporters of the channel through YouTube Memberships
Images/Videos:
NASA, ESA, and A. Feild (STScI)
Antonio Ciccolella CC BY-SA 4.0 https://en.wikipedia.org/wiki/Local_Group#/media/File:Local_Group_and_nearest_galaxies.jpg
RJHall CC BY-SA 3.0 https://en.wikipedia.org/wiki/RR_Lyrae_variable#/media/File:Rr_lyrae_ltcrv_en.svg
Chris Mihos (Case Western Reserve University)/ESO -CC BY 4.0 https://en.wikipedia.org/wiki/Virgo_Cluster#/media/File:ESO-M87.jpg
ESO/VVV Survey/D. Minniti - https://www.eso.org/public/images/eso1636a/ CC BY 4.0
Licenses used:
https://creativecommons.org/licenses/by/4.0/
https://creativecommons.org/licenses/by-sa/4.0/
https://creativecommons.org/licenses/by/3.0/
https://creativecommons.org/licenses/by-sa/3.0/
https://creativecommons.org/licenses/by/2.5/
https://creativecommons.org/licenses/by-sa/2.5/
https://creativecommons.org/licenses/by/2.0/
https://creativecommons.org/licenses/by-sa/2.0/
0:56
The Mysteries Of The Galactic Halo!
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-min...
published: 23 Apr 2023
The Mysteries Of The Galactic Halo!
The Mysteries Of The Galactic Halo!
- Report rights infringement
- published: 23 Apr 2023
- views: 189
The galactic halo is a mysterious region surrounding our Milky Way galaxy. In this one-minute video, we explore the mysteries of this ancient and enigmatic part of our universe. We delve into the origin and nature of the galactic halo, including its unique properties and the mysteries it holds. Through stunning visuals and expert insights, we investigate the possibility of dark matter and other unknown elements that exist within the halo. Ultimately, the video portrays the galactic halo as a place of immense curiosity and potential discovery, where we may find answers to some of the most fundamental questions of our existence. Join us on this journey to explore the mysteries of the galactic halo and unlock the secrets of our universe.
9:13
Milky Way Halo Is 1000 Times Hotter Than Sun's Surface
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6
Or get a shirt: https://teesp...
published: 13 Jun 2020
Milky Way Halo Is 1000 Times Hotter Than Sun's Surface
Milky Way Halo Is 1000 Times Hotter Than Sun's Surface
- Report rights infringement
- published: 13 Jun 2020
- views: 83490
You can buy Universe Sandbox 2 here: http://amzn.to/2yJqwU6
Or get a shirt: https://teespring.com/stores/whatdamath
Hello and welcome! My name is Anton and in this video, we will talk about new research that discovered that the halo of the milky way galaxy is ridiculously hot.
Originally presented here: https://aas.org/meetings/aas236
Support this channel on Patreon to help me make this a full time job:
https://www.patreon.com/whatdamath
Space Engine is available for free here: http://spaceengine.org
Enjoy and please subscribe.
Twitter: https://twitter.com/WhatDaMath
Facebook: https://www.facebook.com/whatdamath
Twitch: http://www.twitch.tv/whatdamath
Bitcoins to spare? Donate them here to help this channel grow!
1GFiTKxWyEjAjZv4vsNtWTUmL53HgXBuvu
Alternatively, PayPal donations can be sent here: https://www.paypal.com/cgi-bin/webscr?cmd=_s-xclick&hosted_button_id=DNKM9SDWU3B3Q&source=url
The hardware used to record these videos:
CPU: https://amzn.to/2LZFQCJ
Video Card: https://amzn.to/2M1W26C
Motherboard: https://amzn.to/2JYGiQQ
RAM: https://amzn.to/2Mwy2t4
PSU: https://amzn.to/2LZcrIH
Case: https://amzn.to/2MwJZz4
Microphone: https://amzn.to/2t5jTv0
Mixer: https://amzn.to/2JOL0oF
Recording and Editing: https://amzn.to/2LX6uvU
Some of the above are affiliate links, meaning I would get a (very small) percentage of the price paid.
Thank you to all Patreon supporters of this channel
Specifically, great thanks to the following members:
Morrison Waud
Vlad Manshin
Mark Teranishi
TheHuntress
Ralph Spataro
Albert B. Cannon
Lilith Dawn
Greg Lambros
adam lee
Gabriel Seiffert
Henry Spadoni
J Carter
Jer
Silver surfer
Konrad Kummli
Nick Dolgy
UnexpectedBooks.com
Mario Rahmani
George Williams
Shinne
Jakub Glos
Johann Goergen
Jake Salo
LS Greger
Lyndon Riley
Lauren Smith
Michael Tiganila
Russell Sears
Vinod sethi
Dave Blair
Robert Wyssbrod
Randal Masutani
Michael Mitsuda
Assaf Dar Sagol
Liam Moss
Timothy Welter MD
Barnard Rabenold
Gordon Cooper
Tracy Burgess
Douglas Burns
Jayjay Volz
Anataine Deva
Kai Raphahn
Sander Stols
Bodo Graßmann
Daniel Charles Smith
Daniel G.
Eugene Sandulenko
gary steelman
Max McNally
Michael Koebel
Sergio Ruelas
Steven Aiello
Victor Julian Castillo
xyndicate
Honey Suzanne Lyons
Olegas Budnik
Dale Andrew Darling
Niji
Peter Hamrak
Matthew Lazear
Alexander Afanasyev
Anton Newman
Anton Reed
0:47
Probing a galactic halo with Hubble
This animation shows the method used to probe the gas around distant galaxies. Astronomers...
published: 25 Apr 2013
Probing a galactic halo with Hubble
Probing a galactic halo with Hubble
- Report rights infringement
- published: 25 Apr 2013
- views: 1586
This animation shows the method used to probe the gas around distant galaxies. Astronomers can use tools such as Hubble's Cosmic Origins Spectrograph (COS) to probe faint galactic envelopes by exploiting even more distant objects — quasars, the intensely luminous centres of distant galaxies powered by huge black holes.
As the light from the distant quasar passes through the galaxy's halo, the gas absorbs certain frequencies -- making it possible to study the region around the galaxy in detail.
This new research utilised Hubble's COS to peer through the very thin outskirts of galactic halos, much further out than shown in this representation, to explore galactic gas at distances of up to twenty times greater than the visible size of the galaxy itself.
More information and download-options:
http://www.spacetelescope.org/videos/heic1308a/
Credit:
ESA, NASA, L. Calçada
4:58
Halo 4 OST - To Galaxy
Tenth track of the Halo 4 Original Soundtrack
published: 10 Nov 2012
Halo 4 OST - To Galaxy
Halo 4 OST - To Galaxy
- Report rights infringement
- published: 10 Nov 2012
- views: 509171
Tenth track of the Halo 4 Original Soundtrack
5:03
To Galaxy
Provided to YouTube by Republic of Music
To Galaxy · Halo · Neil Davidge
Halo 4
℗ Micro...
published: 14 Apr 2023
To Galaxy
To Galaxy
- Report rights infringement
- published: 14 Apr 2023
- views: 14581
Provided to YouTube by Republic of Music
To Galaxy · Halo · Neil Davidge
Halo 4
℗ Microsoft Studios
Released on: 2012-10-19
Auto-generated by YouTube.
3:36
Andromeda Has A Supermassive Halo
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive...
published: 12 Sep 2020
Andromeda Has A Supermassive Halo
Andromeda Has A Supermassive Halo
- Report rights infringement
- published: 12 Sep 2020
- views: 2364
In a recent study, using NASA’s Hubble Space Telescope, scientists mapped the supermassive halo of gas surrounding the Andromeda galaxy. The halo is so big it's interacting with the Milky Way's halo.
Source: https://iopscience.iop.org/article/10.3847/1538-4357/aba49c
Support us on Patreon and help Cosmoknowledge become the number one destination for science: https://www.patreon.com/cosmoknowledge
SUBSCRIBE ► https://goo.gl/PLLFPz
----
Website ► https://cosmoknowledge.com/
TikTok ► https://www.tiktok.com/@cosmoknowledge
Instagram ► https://www.instagram.com/itscosmoknowledge
Facebook ► https://facebook.com/cosmoknowledgee
Edited by:
Ardit Bicaj
Narrated by:
Russell Archey
https://www.ravonmedia.com/
Graphics & Credits:
Space Engine
Universe Sandbox 2
NASA, ESA, J. DePasquale and E. Wheatley (STScI), and Z. Levay
Music:
Close Encounter - Wendel Scherer
Thank you to our Patrons:
DonPig
-
Cosmoknowledge brings news from space.
We love you, explorers!
Halo-
Halo- is a Greek prefix meaning "salt." In biology, it is often used to indicate halotolerance and is a portion of many words:
See also
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Halo-
Classroom Aid - The Galactic Halo...
Teach Astronomy - Galactic Halo...
Galactic Disk Structure | Milky way rotation curve...
Most Distant Halo Stars in Milky Way Are Halfway t...
The Mysteries Of The Galactic Halo!...
Milky Way Halo Is 1000 Times Hotter Than Sun's Sur...
Probing a galactic halo with Hubble...
Halo 4 OST - To Galaxy...
To Galaxy...
Andromeda Has A Supermassive Halo...
Latest News for: galactic halo
Edit
High Velocity Clouds Comprise Less of the Milky Way’s Mass Than We Thought
Edit
Globular Clusters Evolve in Interesting Ways Over Time
Globular clusters are among the oldest objects in the Universe ... Globular clusters are dense, spherical collections of stars that orbit the outer regions of galaxies, usually in the galactic halo ... M13 – Credit. R. Jay GaBany ... Image Credit. ESO ... .
Edit
A Star Was Kicked Out of a Globular Cluster by an Intermediate-Mass Black Hole
Edit
Giant Bubbles Appear To Be Coming From Our Galaxy's Supermassive Black Hole
Edit
New measurements reveal the enormous halos that shroud all galaxies in the universe
photo: NASA, J. Olmsted (STScI)
SPACE NEWS: NASA’s Nancy Grace Roman Space Telescope to Investigate Galactic Fossils
Edit
NASA's Roman Space Telescope to investigate galactic fossils
However, due to the sheer size of galactic halos (they are often 15–20 times as big as the galaxy itself), current telescopes are deeply inefficient at observing them.
Edit
Astronomers explore the nature of galaxy NGC 891 with JWST
Trying to explain the survival of dusty material for several tens of million years after having been ejected by galactic winds in the disk-halo interface, the astronomers offer the two most plausible scenarios.
Edit
New study uses self-interacting dark matter to solve the final parsec problem
Edit
Astrophysicists uncover supermassive black hole/dark matter connection in solving the 'final parsec problem'
... cloud or halo in which they are embedded ... For example, the researchers found that the interactions between dark matter particles they modeled also explain the shapes of galactic dark matter halos.
photo: NASA, Joseph Olmsted (STScI)
Observations Of Distant Galaxies Throw Up New Mystery For Dark Matter
Edit
Mapping the Milky Way’s Dark Matter Halo
Galaxies rotate just like a spinning top and the galactic disk experiences precession or a wobble due to the torque forces from the surrounding dark matter halo.
- 1
- 2
- Next page »