Live from AAS 2018: The Latest News from NASA Astrophysics
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Science Briefing January 11, 2018 Dr. Enrique Lopez-Rodriguez (SOFIA Science Center) Live from AAS 2018: Dr. Francisco Muller-Sanchez (CU-Boulder) Dr. Geert Barentsen (NASA Ames) The Latest News from NASA Astrophysics Facilitators: Dr. Brandon Lawton (STScI) James Manning (UoL)
Additional Resources http://nasawavelength.org/list/2005 Exhibits/Multimedia: ViewSpace – New Interactive Explorations of Multiwavelength Observations Visualization: New Orion Visible/IR Fly-Through Universe Unplugged: New Celebrity Videos Immersive Experiences: Cassiopeia A Supernova Remnant – New Simulation and 360 Degree Video 360 Degree Video: New Visualization of the Galactic Center 2
Black Hole Double Burp new burp old burp Francisco Muller Sanchez University of Colorado, Boulder Additional authors: Julie Comerford, Scott Barrows, Rebecca Nevin, Jenny Greene, 10 David Pooley, Daniel Stern, Fiona Harrison
When Black Holes Burp When a supermassive black hole feeds, it also expels energy in the form of a “burp” Supermassive black hole = found at the center of a galaxy, weighs a million to a billion times the Sun 11 Black Hole Double Burp
When Black Holes Burp When a supermassive black hole feeds, it also expels energy in the form of a “burp” Supermassive black hole = found at the center of a galaxy, weighs a million to a billion times the Sun 12 Black Hole Double Burp
Our Discovery: A Double Burp We discovered a black hole with two burps in the galaxy SDSS J1354+1327, new burp: extends located 800 million lightyears away 3,000 lightyears black hole old burp: This image shows data from the extends 30,000 Hubble Space Telescope and lightyears Chandra X-ray Observatory (pink) Black Hole Double Burp 13
A Galactic Food Coma The new burp is moving like a shock wave, similar to a sonic boom new burp: extends 3,000 lightyears black hole 100,000 years between the two burps old burp: extends 30,000 lightyears This black hole feasted, burped, and napped, then feasted and burped again Black Hole Double Burp 14
Why Is This Important? Theory predicts that black holes flicker on and off when they eat separate meals This galaxy is the strongest evidence that black holes do flicker on timescales much shorter than the age of the Universe (14 billion years) 15 Black Hole Double Burp
Simulations: Observations: new burp new burp old burp old burp Gabor & Bournaud 2013, 2014 16 Black Hole Double Burp
Why Are There Two Burps? Because the black hole had two separate feasts 17 Black Hole Double Burp
Why Are There Two Burps? Because the black hole had two separate feasts A collision between J1354 and another galaxy (40,000 lightyears away) caused material to swirl towards J1354’s black hole This material was eaten as two separate snacks, leading to two burps 18 Black Hole Double Burp
Why Did We Find the Double Burp? When we looked at the spectrum of light from J1354, we saw that the velocity of gas associated with the black hole was 160,000 mph different than the velocity of everything else in the galaxy Got more observations to find out why The 160,000 mph gas was coming from the shock wave from the new burp, and we were lucky to still see the old burp before it fades away 19 Black Hole Double Burp
A Burp Closer to Home Another team found that our Milky Way’s supermassive black hole had a single burp millions of years ago Right now our Galaxy’s black hole is napping, but maybe it will feast and burp again! see Su, Slatyer, & Finkbeiner 2010 20 Black Hole Double Burp
A Near-Resonant Chain of Five Sub-Neptune Planets Found by Citizen Scientists Geert Barentsen • NASA Kepler/K2 Jessie Christiansen • Caltech/IPAC-NExScI Geert.Barentsen@nasa.gov @GeertHub 21
Problem: The NASA K2 mission is too successful! K2 uses the Kepler spacecraft to look for exoplanets Every 3 months K2 releases ~100 million new observations, which need to be calibrated, cleaned up, and searched for signatures of planets Then potential planet signals need to be examined to find the best candidates Then those candidates need to be confirmed or rejected as real planets via extensive additional observations… ... astronomers are swamped! 22
Solution: Citizen scientists! is a public platform for hosting citizen science projects We made exoplanetexplorers.org to get help examining candidates (PI Ian Crossfield) 23
Solution: Citizen scientists! is a public platform for hosting citizen science projects We made exoplanetexplorers.org to get help examining candidates The project was launched by Stargazing Live (BBC/ABC) on live, prime-time television 24
Solution: Citizen scientists! is a public platform for hosting citizen science projects We made exoplanetexplorers.org to get help examining candidates The project was launched by Stargazing Live (BBC/ABC) on live, prime-time television In 48 hours, … and found 10,000 volunteers made 2 million over 180 new classifications… planet candidates! 25
Solution: Citizen scientists! is a public platform for hosting citizen science projects We made exoplanetexplorers.org to get help examining candidates The project was launched by Stargazing Live (BBC/ABC) on live, prime-time television In 48 hours, … and found 10,000 volunteers made 2 million ✘✘✘✘ ✘✘✘✘ ✘✘✘✘ over 180 new ✘✘✘✘✘ ✘✘✘✘✘ ✘✘✘✘✘ classifications… ✘✘✘ ✘✘✘ ✘✘✘ planet candidates! 26
Introducing K2-138 A very compact system of (at least!) five sub-Neptune planets 27
Introducing K2-138 Each year = 12.5 days Each year = 2.5 days A very compact system of (at least!) five sub-Neptune planets 28
A Special Spacing… 3:2 (1.5) 29
A Special Spacing… 3:2 (1.5) 1.513 30
A Special Spacing… 3:2 (1.5) 1.513 1.518 31
A Special Spacing… 3:2 (1.5) 1.513 1.518 1.528 32
A Special Spacing… 3:2 (1.5) 1.513 1.518 1.528 1.544 33
A Special Spacing… K2-138 has the longest chain 3:2 (1.5) 1.513 1.518 1.528 1.544 found close to this type of fundamental resonance These resonant chains give us important clues as to how planets form and migrate 34
The Music of the Spheres 3:2 (1.5) 1.513 1.518 1.528 1.544 35
The Music of the Spheres 3:2 (1.5) 1.513 1.518 1.528 1.544 36
“greater The Music of the Spheres imperfect fifth” 3:2 (1.5) 1.513 1.518 1.528 1.544 37
Summary Citizen scientists using exoplanetexplorers.org discover a near-resonant chain of five sub-Neptunes K2-138, like TRAPPIST-1, may represent a pristine chain of resonances indicative of slow, inward disk migration Kepler data will continue to yield discoveries for years to come. We are uploading three new batches of potential planet signals to exoplanetexplorers.org today! 38
ViewSpace https://viewspace.org/ New Interactive Features 39
Visualization: New Orion Fly-through http://hubblesite.org/video/1003/science 40
Universe Unplugged: Celebrity Videos https://www.ipac.caltech.edu/outreach/project/universe-unplugged 41
Simulation: Cassiopeia A Supernova Remnant http://smithsonianeducation.org/interactives/cassiopeia/index.html 42
Visualization: An Immersive Tour of the Galactic Center https://youtu.be/YKzxmeABbkU 43
Links to science press releases at: aas.org/meetings/aas231/press-kit Some Sloan Digital Sky Survey-based results: • Robert Wilson – Iron-rich stars host short-period (“hot”) planets. • Catherine Grier – Using “reverberation mapping” to measure masses of supermassive black holes in AGNs. • Karen Masters – Finding evidence of supermassive black holes even in some dwarf galaxies. Dennis Bodewits – Comet 41P/Tuttle-Giacobini-Kresak dramatically slowed its rotation probably due to jets. Jay Lockman – Hot, small hydrogen clouds detected in Fermi Bubbles. Christopher Russell – Immersive visualization of galactic center from perspective of Sgr A. Renske Smit – “Whirpool” motion detected a two galaxies 800 M years after Big Bang, suggesting some of the earliest galaxies “matured” quickly. 44
Links to science press releases at: aas.org/meetings/aas231/press-kit Keith Gendreau – ISS-stationed NICER X-ray instrument successfully demonstrated the concept of using millisecond pulsars as deep space navigation beacons, triangulating its position to within 10 km. William Clarkson – Used HST archival data to chart proper motions of Galactic Bulge sun-like stars – found metal-rich populations moving differently (faster) than metal-poor stars. Julie Comerford – Found a galaxy whose central black hole shows a “double burp” of high-energy particles from separate episodes of “feasting”—showing that black holes “flicker” on and off in this way on relatively short times scales. Brett Salmon – Used gravitational lensing to find a small, “embryonic” galaxy formed just 500 million years after the Big Bang. 45
Fast Radio Burst 121102: Betsy Adams, Andrew Seymour, Vishal Gajjar, Daniele Michilli, Jason Hessels • Presently unique FRB in that it repeats. • Located 3 billion LY away, in star-forming region of a dwarf galaxy. • Associated with a persistent radio source. • Radio signal has structure. • Emission region is less than 10 km across (neutron star?). • Exists in an extreme magnetic environment. • Possible models: neutron star near massive black hole, or in a very bright nebula. 46
Adam Reiss: Do new measurements of the expansion rate of the universe suggest evidence for new physics? arxiv.org/abs/1604.01424 • Refined parallax measurements of nearby Cepheid variables using HST; used the results to refine the “distance ladder” to reduce the error bars in the measurement of the “local” Hubble Constant to 2.4%. (73.2 km/sec/Mpc) • Continued difference with the Planck-derived number from the early universe. (66.9 km/sec/Mpc) • Is this evidence for a difference in the physics of the early universe compared to the later? • Shooting for a 1% error level in the future to constrain the cosmological model. 47
To ensure we meet the needs of the education community (you!), NASA’s UoL is committed to performing regular evaluations, to determine the effectiveness of Professional Learning opportunities like the Science Briefings. If you prefer not to participate in the evaluation process, you can opt out by contacting Kay Ferrari . This product is based upon work supported by NASA under award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Jet Propulsion Laboratory, Smithsonian Astrophysical Observatory, and Sonoma State University. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. 48
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