Space Physics and Astronomy Dr. Darrel Smith, Chair Department of Physics College of Arts & Sciences Temasek Polytechnic Visit September 6, 2013.

Slides:



Advertisements
Similar presentations
Observation of the Universe from the Moon – Elisabetta Cavazzuti – LNF May 7, 2007 ITALIAN VISION FOR MOON EXPLORATION OBSERVATION OF THE UNIVERSE FROM.
Advertisements

Northern Michigan University Department of Physics.
The Need for Speed Dr. Darrel Smith, Chair Space Physics August 27, 2005 Dr. Darrel Smith, Chair Space Physics August 27, 2005.
The Very Large Array Past and Future Dave Finley.
LIGO-G W "Colliding Black Holes" Credit: National Center for Supercomputing Applications (NCSA) LIGO for Chemists Fred Raab, LIGO Hanford Observatory.
1 Science Opportunities for Australia Advanced LIGO Barry Barish Director, LIGO Canberra, Australia 16-Sept-03 LIGO-G M.
LIGO-G W Measuring Ripples in the Geometry of Space Fred Raab LIGO Hanford Observatory.
Laser Interferometer Space Antenna Satellite Description  Three spacecrafts forming a triangle flying 5 million km apart  Placed in an elliptical plain.
2/9/2006Welcome to LIGO1 Welcome to LIGO!. 2/9/2006Welcome to LIGO2 LIGO: A detector that measures very tiny displacements How tiny?
Welcome to the Department of Physics at the Rochester Institute of Technology.
LIGO-G W What If We Could Listen to the Stars? Fred Raab LIGO Hanford Observatory.
Two Supermassive Black Holes in the Same Galaxy. Profile of the Galaxy – NGC Discovered by NASA’s Chandra X-ray Observatory - Nucleus of the galaxy.
Laser Interferometer Gravitational-Wave Observatory Who? Presented By: Bonnie Wooley.
1 Observing the Most Violent Events in the Universe Virgo Barry Barish Director, LIGO Virgo Inauguration 23-July-03 Cascina 2003.
LIGO-G W Measuring Ripples in the Geometry of Space Fred Raab LIGO Hanford Observatory.
The LIGO Project ( Laser Interferometer Gravitational-Wave Observatory) Rick Savage – Scientist LIGO Hanford Observatory.
Michigan Math and Science Scholars Lunch and Learn Series 2005.
LIGO -- Studying the Fabric of the Universe LIGO-GOxxxx Barry C. Barish National Science Board LIGO Livingston, LA 4-Feb-04.
What are Gravity Waves?. According to Einstein's theory of gravity, an accelerating mass causes the fabric of space-time to ripple like a pond disturbed.
Careers in Astronomy. A Future in Astronomy So you want to be an astronomer, but what do you need to do now to get there? –Get involved in research and.
Mid-Atlantic Regional Space Grant Meeting – October 1-2, Astronomy and Space Science Project Proposal New Jersey Space Grant Consortium Dr. Siva.
Introducing Astronomy Education into High School Physics Curriculum Through the Use of the University of North Dakota Observatory Caitlin Nolby Space Studies.
Careers in Astronomy AST 200. Astronomy Primary Goal: Understanding the nature of the universe and its constituents Means: Equipment building, research,
25 Years of the Hubble Space Telescope A Celestial Silver Celebration Dr. Frank Summers Space Telescope Science Institute February 5, 2015.
Teória relativity začiatok alebo koniec fyziky.
CPEP and Gravitation Lynn Cominsky Sonoma State University.
1 LIGO Education and Outreach Gregory Harry On behalf of the LIGO Scientific Collaboration’s Education and Public Outreach Working Group Joint Spring Meeting.
ERAU Space Sciences Program1 A New Bachelor of Science Degree in the College of Arts & Sciences By Dr. Nick Devereux And Dr. Darrel Smith.
J. D. Cline, M. W. Castelaz Pisgah Astronomical Research Institute PARI Education and Research Programs Session 2.02 Monday, May 30, AAS 206th Meeting.
Gravitational Wave Arezu Dehghafnar Physics Department SUT.
LIGO-G L LIGO Livingston Observatory Mark Coles Observatory Head LIGO Livingston Observatory California Institute of Technology.
Acknowledgements The work presented in this poster was carried out within the LIGO Scientific Collaboration (LSC). The methods and results presented here.
Gravitational Interactions
To do this, we need to make a model.
Chapter 18 Life In The Universe. We have already launched our first robotic spacecraft into interstellar space Pioneers 10 and 11 carry a copy of this.
Prospects for observing quasar jets with the Space Interferometry Mission Ann E. Wehrle Space Science Institute, La Canada Flintridge, CA, and Boulder,
Center for Astronomy. Vision & Objectives Maintain the number 1 status in Korea. Aim to be a world-class astronomy institute. Regarding Yonsei-Oxford.
Possibility of detecting CHRISTODOULOU MEMORY of GRAVITATIONAL WAVES by using LISA (Laser Interferometer Space Antenna) Thus, the final form of the memory.
DEPARTMENT OF PHYSICS AND ASTRONOMY Professor Bob Warwick Head of Department.
© Sierra College Astronomy Department 1 Astronomy 10 Elementary Astronomy COURSE GOALS & OBJECTIVES.
Loose ends and Magnetic Fields in Astronomy - Exam tips – come to class! - Course Evaluations – come to class! - energy in fields - magnetism in matter.
Structure Formation in the Universe Concentrate on: the origin of structure in the Universe How do we make progress?How do we make progress? What are the.
LIGO-G Z LIGO at the start of continuous observation Prospects and Challenges Albert Lazzarini LIGO Scientific Collaboration Presentation at NSF.
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 13. Gravitational waves.
More to the universe than meets the eye
Space Physics Astrophysics Dr. Brent Buckalew, Dr. Nick Devereux, Dr. Brian Rachford, Particle Physics & Cosmology Dr. Darrel Smith, Dr. Quentin Bailey,
Physics – The Beginning. What is Physics? Physics is a natural science that studies the behavior and structure of matter and energy. Physics is a natural.
LIGO-G v5 5/2/09Joshua Smith, Syracuse University1 Low-latency search for gravitational-wave transients with electromagnetic follow-up Joshua Smith,
Big Bang Related Websites: 4- Cosmology; Black Holes and Big Bang Particle Make-up of the Atom.
The Search for Black Holes
Search terms: REU (NSF supported summer programs at Universities around the country) SULI (DOE supported programs at National Labs – summer and academic.
LIGO-G M Scientific Operation of LIGO Gary H Sanders LIGO Laboratory California Institute of Technology APS Meeting APR03, Philadelphia Gravitational-Wave.
ERAU Space Physics Program1 Space Physics Program College of Arts & Sciences ERAU-Prescott Dr. Darrel Smith World Space Congress October 17, 2002.
LIGO-G M Press Conference Scientific Operation of LIGO Gary H Sanders Caltech (on behalf of a large team) APS April Meeting Philadelphia 6-April-03.
ASP2011 Measurement Techniques Lectures 7-8 Dr. Duncan Galloway University of Melbourne
The Search for Black Holes
Steering Astronomy Toward Gravitational Wave-Supernova Science Kiranjyot (Jasmine) Gill, 1 Dr. Michele Zanolin 1 With support from Marek Szczepanczyk 1.
LIGO Educational Outreach: The Science Education Center
LIGO at a Distance Dale Ingram on behalf of the LIGO Laboratory Public Outreach Team LIGO Hanford Observatory, Richland, WA
LIGO: Laser Interferometer Gravitational-wave Observatory
Chandra Science Highlight
Astrophysics: 2016 highlights and the way forward
Is there a future for LIGO underground?
LIGO detectors: past, present and future
DIRECT DETECTION OF GRAVITATIONAL WAVES FROM NEUTRON STARS
A Galaxy Revealed in Multiple Wavelengths
Quasars.
Solar Physics and the Total Solar Eclipse of 2017 August 21
The Laser Interferometer Gravitational-Wave Observatory
Life as an Astronomer: 1. What do Astronomers Study?
Presentation transcript:

Space Physics and Astronomy Dr. Darrel Smith, Chair Department of Physics College of Arts & Sciences Temasek Polytechnic Visit September 6, 2013

Areas of Undergraduate Research 1. Astronomy 2.Gravitational Physics/Cosmology 3. Space Propulsion Systems 4. Particle Astrophysics / LIGO On the web:

Summer Internships The MiniBooNE Detector At Fermilab

MiniBooNE Collaboration at Fermilab

Gravitational Waves sensing with LIGO LIGO Livingston Observatory LIGO Hanford Observatory "Colliding Black Holes“ Credit: National Center for Supercomputing Applications (NCSA) Dr. Andri Gretarsson Dr. Brennan Hughey Dr. Michele Zanolin

The LIGO Experiment

Relativity violations imply a modified acceleration on Earth Atom interferometers can measure daily changes in the local gravitational acceleration on Earth arising from violations of the laws of Relativity. This was recently studied by a group of Stanford physicists using atom interferometers.

Dr. Darrel Smith Exotic Propulsion Lab (Bldg. 56) Nuclear thermal propulsion (simulation only) Matter-antimatter propulsion Arc jet thruster Pulsed plasma thruster (PPT) Goal: Measure the specific thrust of different exotic propulsion engines Areas of Concentration Exotic Propulsion

 Pulsed Plasma Thrusters (PPTs) Zachery Northern Exotic Propulsion at ERAU Prescott  Matter-Antimatter Propulsion Matt Boyd  Nuclear Thermal Propulsion (NTP) Theoretical Modeling Steven Walton

Areas of Concentration Space Propulsion Systems (cont’d) Nuclear Thermal Propulsion Antimatter Engines Ion-Compressed Antimatter Nuclear Engine Total Mission Duration (Days with 30 days on Surface)

Road Trips (Los Alamos Nat’l Lab) Road Trips (JPL--Pasadena, CA) 1.Society of Physics Students 2.Sigma-Pi-Sigma (Honors Society) Road Trips

Road Trips (JPL--Pasadena, CA)

Space Physics Program On the web: This is a 4-year program. 120 credit hours You will want to average ~15 credit hours per semester. Many students are involved in undergraduate research projects before their senior year.

Astronomy Program (New Program) 1.Starting Fall Combination of Astronomy and Astrophysics 3.Dr. Brian Rachford (Program Chair)

Astronomy Program Undergraduate Research Projects 1.Funded Hubble Space Telescope (NASA) Search for super–massive black holes, and galaxy formation. 2.Kepler Project (Caltech) Search for extra-solar planets 3.Diffuse Interstellar Bands (DIBs) in collaboration with CU Boulder, Univ. of Chicago and other institutions. Dr. Brian Rachford (Program Chair) Dr. Nick Devereux

Astronomy Program Our Observatory (Variable light sources) 1.Extra-Solar Planets 2.Eclipsing Binary Stars 3.Variable Stars (varying light output-intrinsic to the star) Dr. Brian Rachford (Program Chair) Dr. Nick Devereux

Astronomy Program Research Experience for Undergraduates (Summer) 1.NSF supported REU summer internships 2.NASA supported summer internships Program is already developed inside the Space Physics program 1.Students have already published in peer-reviewed journals. 2.Observatory, Radio Telescopes, and antenna arrays are already up and running.

Physics and Astronomy 1.Prepare students for jobs in industry and labs. 2.Prepare students for graduate school Graduate Records Exams (GREs)