
Dr. Brian Thomas leads the research
team studying astrobiophysics (also called astrobiology) in
the Department of Physics and Astronomy at Washburn University. Our
group works on several different projects which study the
impact on the Earth by radiation from space. Details of some
projects can be found below.
Astrobiophysics studies
the effect of astrophysical processes of life on Earth, as
well as effects on possible life elsewhere.
We distinguish it from astrobiology, which is concerned with
finding extraterrestrial life. To do this work, a wide
variety of research areas which include astrophysics,
astronomy, biochemistry, evolutionary biology,
paleontology, atmospheric science, and a host of others are
combined.
The Washburn
Astrobiophysics group's primary research tool is computational
modeling. This modeling makes use of the Washburn High
Performance Academic Computing Envrionment, HiPACE.
Our current focus is a NASA funded project entitled "Astrophysical Ionizing Photon Events and Primary Productivity of Earth's Oceans." Dr. Thomas is the principal investigator of this project and it is being conducted in collaboration with Dr. Adrian Mellott at the University of Kansas and Dr. Patrick Neale at the Smithsonian Environmental Research Center. The purpose of the project is two-fold:
Our work in the area began in 2003 with an exploration of the effect on the Earth radiation (X-Rays & Gamma-Rays) from a gamma-ray burst in our galaxy. From there it has expanded and diversified. Dr. Thomas and the Washburn Astrobiophysics group have been heavily involved the following projects in collaboration with the KU Astrobiophysics Working Group.
Please see the Working Group's website for more: http://kusmos.phsx.ku.edu/~melott/Astrobiology.htm
I.
Astrophysical Ionizing Radiation Events--the Effect
on Our Biosphere:
Large explosions in the Sun’s atmosphere called Solar Flares emit X-Rays & UV-Radiation. There are also occasional much more powerful flares. Stars with an 8 solar mass or greater create supernovae. A Supernova is created once every 50 years. Earth would have to be within a 10 Light Year Radius of the blast for the affect to be disastrous by. A star that has a mass 30 times or greater than our Sun creates a Hypernova, which is 10 times more powerful than a typical Supernova. The core collapses into a Black Hole. Two energetic jets of plasma are emitted from the star’s rotational poles along the dying star’s axis at nearly the speed of light producing an intense long-duration Gamma-Ray Bursts (GRBs). A GRB 6,500 light years away from Earth could cause potentially severely damaging events likely on a timescale of a few hundred million years. Our first efforts, and still the most prolific, lie in this area. In the sections below, we explore several different likely or possible kinds of radiation events and their effects on the Earth.
Through atmospheric
modeling, we have estimated that a Gamma Ray Burst could have
contributed to the Ordovician extinction
450 million years ago; 60% of all marine invertebrates were
lost. An ice age is thought to have caused
this extinction, however, a Gamma-Ray Burst could have caused a
fast die-out early on and also could have triggered the significant
drop in surface temperature on Earth. Scientists
calculated that Gamma-Ray radiation from a relatively
nearby star explosion, hitting the Earth for only ten
seconds, could deplete up to half of the atmosphere's
protective ozone layer. Recovery could take at least
five years.
We
have conducted a study of the atmospheric chemistry effects of
comets, especially as related to the hypothesis that the Clovis
culture and North American megafauna may have been killed off by a
comet impact 12,900 years ago. See here for more
information:
Our
Study of Comets and Atmospheric Chemistry
2007
American Astronomical Society workshop "Astrophysical ionizing
radiation sources and their impact on life." For more
information look here.
At the Astrobiology Science Conference, 2008. We organized
one of the 39 parallel sessions. Two of the talks pegged
as most exciting in a review by Astrobiology
Magazine were in our session: The
Habitable
Galaxy
Some of our work was featured prominently in a
National Geographic Television program entitled
"Extinctions." The program will be rebroadcast periodically.
Research in our group constituted approximately the last
third of the program. Their summary: "Planet earth
teems with life, but imagine it disappearing in one go: a victim
of catastrophic events that leave the planet almost uninhabitable.
Naked Science travels back in time to examine three of the
largest mass extinctions that decimated life on the planet in the
past. What caused these wipe-outs and could they happen
again in the future, threatening our very survival? Worse
still, are we already in the middle of a mass extinction--not one
created by nature, but by man? This program unravels the
clues and likely suspects behind the dinosaur, Permian, and late
Ordovician wipe-outs. Even given human adaptability and know-how,
would we fare any better than the previous victims of these
disasters? Could we be wiped out? "We discover that we
are not as safe as we'd like to think."
A History Channel presentation features our research. This hour long science special on the destructive potential of gamma-ray bursts was on Megadisasters. It is repeated occasionally on the History Channel. The science content is solid, in spite of the hype surrounding the series as a whole.
Our group has been involved with the Astrobiophysics
Seminar
at KU.
Opportunities exist for students to be involved in
research. Contact Dr. Thomas for more information:
brian.thomas @ washburn.edu
We have a block
of supercomputer time at the National Center for
Supercomputer Appications for those computations too large for local
workstations.
We maintain an active net of collaborators especially
including NASA Goddard
Space
Flight Center, in their Astroparticle
Physics Laboratory and their Laboratory
for Atmospheres. We have an active
project with the Photobiology and Solar Radiation Lab at the Smithsonian
Environmental Research Center. The SWIFT
mission is providing new information about Gamma-ray
bursts, including much-needed data on their rate in the "recent"
Universe (since the Earth formed.)
Our recent research publications can usually be found in
the ArXiv.
Older published research is listed elsewhere.
People:
Washburn University faculty involved in research:
Current and past Washburn student collaborators:
-- Nick VanCamp
-- Brock R. Snyder II
-- Keith Arkenberg
-- Michelle Honeyman
-- Jacob Peterson -- Bianca Lewis
-- Anna Lischke
External Collaborators:
-- KU Astrobiophysics Working Group
Research is Funded by NASA
Design by Bianca L. Lewis
Last Updated: August 18th, 2011
Sources for
Images:
http://www.seeinginthedark.org/images/gallery/exploding_star_gamma.jpg
http://tuttidentro.files.wordpress.com/2009/11/supernova-remnant-cassiopea-a.jpg
http://listverse.files.wordpress.com/2009/08/swift-gamma-ray-lg-tm.jpg
http://www.science.psu.edu/alert/swift-images/SwiftNatureCover.jpg
http://www.columbia.edu/itc/eeeb/baker/N0316/Lecture%205/Images/ordovician.JPG