Dr. Richard Olenick currently serves as Professor of Physics and a teacher of popular
courses in physics and astronomy. He has supervised over fifty undergraduate theses.
His research students have accompanied him to Moscow and to Crimea for observations
of new cataclysmic variable stars as well as to Colorado to gather data to search
for exoplanet transits.
Dr. Olenick served as the Associate Project Director of the PBS television series, The Mechanical Universe and Beyond the Mechanical Universe. He was also principal author of accompanying textbooks published by Cambridge University
Press. He also received numerous grants from the National Science Foundation and
the U.S. Department of Education for the development of curricular material (Comprehensive
Conceptual Curriculum for Physics, C3P) for use in high schools and for workshops for high school physics teachers.
- Cataclysmic Variables
- Accretion Disks
- Exoplanet Searches
- Physics Education
B.S. in Physics, Illinois Institute of Technology
M.S., Ph.D. in Physics, Purdue University
- Professor, University of Dallas
- Fulbright Scholar, Moscow State University
- Adjunct Professor, University of Texas at Dallas
- Research Associate, California Institute of Technology
- Currently Editor for the deGruyter journal Open Physics
- Currently Editor for the BioAccents journal Physics
- Reviewer for the National Science Foundation Graduate Research Fellowship Program
- Reviewer for Open Physics project at Rice University
- Reviewer for Open Astronomy project at Rice University
- Former Committee Member and Item Writer for the Graduate Record Exam Physics Test
- PHY 2303 Physics and Technology
- PHY 3363 Computational Physics
- PHY 2302 Introductory Astronomy
- PHY 4328 Electrodynamics
- PHY 4424 Quantum Mechanics
My research, which was initially funded by the Nancy Cain Marcus and Jeffrey A. Marcus
Chair in Science, involves photometric studies, data analysis, and modeling of cataclysmic
variable stars (CVs). Since then we have discovered and classified a new dwarf
nova, observed exoplanetary transits, and discovered new binaries.
Cataclysmic variables are binary systems in which a white orbits with a normal star.
The orbital periods of CVs typically range from approximately 0.05 day to 0.6 day.
These binaries are quite small by astronomical sizes. The evolution of these binaries
occurs through mass transfer from the secondary to the white dwarf. The luminosity
of CVs is dominated by the accretion disk. Strong tidal forces from the white dwarf
pull hydrogen gas from the surrounding Roche lobe of the secondary and larger star
through the L1 Lagrange point. The gas spirals down around the white dwarf and usually
forms an accretion disk. If the white dwarf has a large magnetic field, the materials
may be directed right onto the surface of the star. As gas accumulates, forming a
shell around the white dwarf, thermonuclear fusion reactions can be re-ignited on
the white dwarf.
My current research into CVs focuses on improved ways of determining the mass ratio
through observations and accretion disk modeling and is carried out with collaborators
Dr. Michele Montgomery at the University of Central Florida and Dr. Irina Voloshina
at the Sternberg Institute of Moscow State University. I take students to Moscow
and Crimea for observations with Dr. Voloshina.
I also search for exoplanets with students and my colleague, Arthur Sweeney in our
STExTS project--Small Telescope Extrasolar Transit Search. Starting in 2011 we set
up telescopes during the summers in Pitkin, Colorado (elevation 9210 ft) and later
in the Upper Peninsular. For the past two years we have used our telescopes at the
Monroe Robotic Observatory of the University of North Texas to gather data. Each
summer we gather data on approximately 3500 - 5000 stars for 30 - 38 nights and then
sift through the light curves looking for transits. We currently have seven candidates
for new exoplanet transits.
During our transit searches we have discovered numerous new stars, many of which are
now listed in the Variable Star Index of the American Association of Variable Star
Observers (AAVSO) and which we are currently writing up for publications. These discoveries
include RR Lyrae stars exhibiting the Blazhko effect and delta Scuti stars.
- “Photometric Observations and Numerical Modeling of SDSS J162520.29+120308.7” with
Michele Montogomery, Irina Voloshina, Kyle Meziere, and Vladimir Metlov, New Astronomy, 50, 43 (2017).
- Evolutionary Paths of AM CV’ns to Supernovae, Grant Proposal submitted 1 November 2016 to NASA, K2 Guest Observer Program Cycle
with M. Montgomery and I. Voloshina.
- EWASS 2017 Session Organizer on "Undergraduate Research in Astronomy", Prague (2017).
- A Comparison of Observations and SPH Modeling of the Outbursts of the WZ Sge-Type
Dwarf Nova SDSS J213806.5+261957, with I. Voloshina, M. Montgomery, J. Rovny, A. Sweeney,
V. Metlov, in preparation for Astronomy and Astrophysics.
- The Superoutburst of SDSS J1625+120308 in July 2010, I. Voloshina, R. Olenick, K. Meziere, V. Metlov, J. Rovny, Proceeding of the Ninth
Pacific Rim Conference on Stellar Astrophysics, Astronomical Society of the Pacific
Conference Series, Vol. 451, p. 195-199 (2011).
- How White Dwarfs Become Supernovae, LeTourneau University Colloquium, 27 October 2016
- Small Telescope Exoplanet Transit Searches, University of North Texas Colloquium, 17 November 2015
- STExTS—Small Telescope Extrasolar Planetary Transit Search, Colloquium at Michigan Technological University. 15 October 2015
- How White Dwarfs Evolve in Supernovae, Colloquium at Northern Michigan University, 14 September 2015
- Haggerty Science Fellow
- King Scholar
- Fulbright Scholar
- Minnie Piper Stevens Professor
- Carnegie Foundation Texas Professor of the Year
- Haggar Scholar