MIfA Public Lecture Series
The Minnesota Institute for Astrophysics is dedicated to bringing the excitement of modern astrophysical research to the Minnesota public.
The MIfA public lecture series, held once per semester, is our way to communicate the exciting research activities of MIfA researchers directly to the public.
Date for the next MIfA Lecture TBD.
Galaxy Clusters: Nature’s Giant Magnifying Glasses
Dr. Patrick Kelly
Galaxy Clusters are vast concentrations of many hundreds of galaxies bound together by gravity. Einstein's theory of general relativity predicts that if light traveling towards us passes close to such a massive object, its path will be bent, and it will take longer for the light to reach us. Indeed, galaxy clusters act as giant and spectacular magnifying glasses that not only magnify background galaxies but also create multiple images of them. Dr. Kelly will talk about what happens when a massive star explodes as a luminous supernova in one of those distant, multiply imaged galaxies. He will also describe a recent discovery that individual stars in galaxies more than halfway across the universe can become so highly magnified by galaxy clusters that we can see them one-by-one from Earth.
Aurora: Mysteries of the Northern Lights
The dancing, shimmering glow of the northern lights, the aurora borealis (and their counterpart in the southern hemisphere, the aurora australis) has amazed mankind for centuries. Early northern peoples from Alaska to Siberia have wondered about the lights and created legends to explain them. Now in the space age, experiments flown on satellites and rockets have shown that the aurora is produced by the impact of electrons on the upper atmosphere and is related to oscillations in the Earth’s magnetic field that are associated with solar activity. The aurora has also been seen at other planets such as Jupiter and Saturn and is likely to be present at planets in other solar systems. This talk will outline our present understanding of the causes of the aurora.
Dark Matter Detectives: Searching for Clues
By the 1990’s there was clear evidence that the Universe was filled with a mysterious form of matter that affected the motion of stars and galaxies, bent light from distant galaxies, and influenced cosmic evolution. While the evidence for the existence of this “dark matter” is overwhelming, its nature is still unknown. Over the last several decades, scientists have been searching for clues, which might reveal how dark matter interacts with normal matter and why there is so much of it. Ever larger experiments have been built deep underground where cosmic rays can’t interfere, in order to capture a glimpse of the elusive dark matter particles as they stream through our solar system. So far, there has not been a confirmed sighting in a terrestrial detector, but the dark matter detectives are not giving up. Learn about what progress has been made over the last decade and where we go from here.
A Walk on the Dark Side
Our Universe is comprised of far more than meets the eye. For 13.8 billion years, gravity has been creating enormous bound structures, the largest of which are clusters of galaxies. Modern telescopes are uncovering an astonishing variety of structures in these clusters which are invisible to the human eye — from X-ray emitting gas at 100s of millions of degrees, to supermassive black holes at the centers of cluster galaxies, to the popularized but not yet understood dark matter that holds everything together. Even the enigmatic dark energy plays a role in cluster formation. Our tour of clusters will start with the first recognition of curious concentrations of fuzzy objects in the sky to the latest discoveries using telescopes across the Earth and space.
Exploring the Mysteries of the Sun: Explosions on our Closest Star
The Sun offers us a special window into the universe, allowing us to study the basic physics at work in many astronomical objects, but it is nearby and relatively easier to measure. Beyond this, there is a practical urgency to understanding the Sun because it is the driver of the space weather that surrounds and affects the Earth. Solar eruptions regularly hit the Earth's magnetic field with large amounts of energy, plasma, and radiation. The origin of these events lies in abrupt releases of magnetic energy on the Sun called solar flares. One of the largest events recorded was the Carrington flare of 1859, which would catastrophically disrupt modern technology if it were to happen today. In this talk, I will describe what we currently know about the physics behind flares and what we hope to learn in the future with new instruments that measure high-energy radiation. I’ll also explore the routes by which telescopes are tested on suborbital platforms before they finally become ready for the limelight aboard a NASA spacecraft.
Observing the Universe with Gravitational Waves
Advanced LIGO gravitational-wave detectors recently recorded the first signals coming from mergers of binary black hole systems, marking the beginning of gravitational-wave astronomy and astrophysics. For the first time we are able to observe and study the universe with gravitational waves, and to learn about objects never observed before. Dr. Mandic will describe the LIGO detectors and the events they recorded, and he will discuss the implications of these observations as well as expectations for future observations.
To the Stars We Will Go — The Worlds of Exoplanets
The recent revolution of exoplanet detections by the NASA Kepler mission and ground-based searches for exoplanets has given way to a new understanding of how common place other worlds are in the Galaxy. Our prospective of astrobiology as suddenly blossomed. Highlighted, as part of this presentation, will be a review of how astronomers detected and characterize these exo-planets, using techniques at the Large Binocular Telescope Observatory and elsewhere, a reflection on the potential requirements of the habitability zones in exo-planetary system, highlights from NASA missions designed to search for alien worlds, and the surprises within our own solar systems of bodies that may harbor life at present of may have supported life in the past. Indeed, we may be at the point where "E.T. will phone home."
To the Zooniverse and Beyond: How Crowdsourcing Science is Solving Big Data Problems in Astronomy
Join Dr. Lucy Fortson, Associate Head and Associate Professor in the School of Physics and Astronomy, as she describes the wildly successful Galaxy Zoo project that led to the birth of the Zooniverse. Along the way, she will describe the issues that researchers now face with “Big Data,” what crowdsourcing is and how it is revolutionizing how science is being done.
Birth of the Universe from the Bottom of the World
At one time the origin and fate of the Universe in which we find ourselves was the subject of speculation by mystics and philosophers. Journey back in cosmic time to the first instant of the Big Bang and learn about the recent evidence for gravitational waves coming from the BICEP2 radio telescope located at the South Pole.