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UID:bb014e0c8a84c82797fc74f7aee8132f
CATEGORIES:Guest Speaker Night
CREATED:20180218T162632
SUMMARY:Guest Speaker - Dr Jesse van de Sande (SIfA, University of Sydney)
DESCRIPTION:<h2>What do galaxies and shadow puppets have in common?</h2><p>Galaxies com
 e in all shapes and sizes. It is hard not to be impressed by the majestic v
 ariety in galaxy morphology that the Universe has to offer. Besides creatin
 g just pretty images, galaxy shape and morphology also provide important cl
 ues on how galaxies formed and evolved. Large computer simulations suggest 
 that collisions between galaxies alter their appearance. The more interacti
 ons a galaxy experiences, the rounder it becomes. However, galaxies are so 
 far away that we can only observe them as two-dimensional projections on th
 e celestial sphere. Figuring out the true shape of galaxies is a bit like s
 hadow puppetry without instructions; ever tried twisting your arms and fing
 ers to create the image of an African Unladen Swallow? So, how do astronome
 rs derive the true three-dimensional shape of galaxies? In this talk I will
  explain how Australian Astronomers have invented an instrument that can do
  exactly that. These tools now allow us to figure out how galaxies like our
  Milky Way have formed and evolve.</p><h2>Dr Jesse van de Sande</h2><p><img
  src="images/articles/Dr_Jesse_van_de_Sande.jpg" alt="Dr Jesse van de Sande
 " style="margin-right: 10px; float: left;" /></p><p>Jesse van de Sande is a
  Research Fellow at the&nbsp;Sydney Institute for Astronomy at the Universi
 ty of Sydney studying how galaxies form and evolve. He tries to solve the b
 ig questions such as &lsquo;How was the Milky Way Galaxy formed?&rsquo; and
  &lsquo;What will happen to our Milky Way after it collides with the Androm
 eda Galaxy?&rsquo; Jesse uses the Anglo Australian Telescope with an instru
 ment called SAMI to study the motions of stars within galaxies. For his PhD
  thesis, he used the Hubble Space Telescope and the Very Large Telescopes i
 n Chilli to investigate the formation and evolution of massive galaxies in 
 the early Universe.&nbsp;</p>
X-ALT-DESC;FMTTYPE=text/html:<h2>What do galaxies and shadow puppets have in common?</h2><p>Galaxies com
 e in all shapes and sizes. It is hard not to be impressed by the majestic v
 ariety in galaxy morphology that the Universe has to offer. Besides creatin
 g just pretty images, galaxy shape and morphology also provide important cl
 ues on how galaxies formed and evolved. Large computer simulations suggest 
 that collisions between galaxies alter their appearance. The more interacti
 ons a galaxy experiences, the rounder it becomes. However, galaxies are so 
 far away that we can only observe them as two-dimensional projections on th
 e celestial sphere. Figuring out the true shape of galaxies is a bit like s
 hadow puppetry without instructions; ever tried twisting your arms and fing
 ers to create the image of an African Unladen Swallow? So, how do astronome
 rs derive the true three-dimensional shape of galaxies? In this talk I will
  explain how Australian Astronomers have invented an instrument that can do
  exactly that. These tools now allow us to figure out how galaxies like our
  Milky Way have formed and evolve.</p><h2>Dr Jesse van de Sande</h2><p><img
  src="https://www.sasi.net.au/images/articles/Dr_Jesse_van_de_Sande.jpg" al
 t="Dr Jesse van de Sande" style="margin-right: 10px; float: left;" /></p><p
 >Jesse van de Sande is a Research Fellow at the&nbsp;Sydney Institute for A
 stronomy at the University of Sydney studying how galaxies form and evolve.
  He tries to solve the big questions such as &lsquo;How was the Milky Way G
 alaxy formed?&rsquo; and &lsquo;What will happen to our Milky Way after it 
 collides with the Andromeda Galaxy?&rsquo; Jesse uses the Anglo Australian 
 Telescope with an instrument called SAMI to study the motions of stars with
 in galaxies. For his PhD thesis, he used the Hubble Space Telescope and the
  Very Large Telescopes in Chilli to investigate the formation and evolution
  of massive galaxies in the early Universe.&nbsp;</p>
DTSTAMP:20260622T124143
DTSTART;TZID=Australia/Sydney:20181004T193000
DTEND;TZID=Australia/Sydney:20181004T213000
SEQUENCE:0
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