Colloquia: Astronomy & Astrophysics colloquia and KICP colloquia - Usually Wednesdays, 3:30 PM, ERC 161, unless otherwise specified. Reception starts at 4:30 PM in Hubble Lounge (Astronomy & Astrophysics colloquia) and ERC 401 (KICP colloquia). Persons with a disability who believe they may need assistance, please call the departmental secretary in advance at 773-702-8203 or email

Current & Future Colloquia
DateTalk TitleSpeaker
April 3, 2019
Astronomy Colloquium
Why doesn't the Solar System have close-in super-Earths?Sean Raymond, Laboratoire d'Astrophysique de Bordeaux, France
April 10, 2019
Astronomy Colloquium
The Search for Biosignature Gases on ExoplanetsSara Seager, MIT
May 1, 2019
Astronomy Colloquium
TBADara Norman
May 15, 2019
Astronomy Colloquium
TBARob Kennicutt
May 29, 2019
Astronomy Colloquium
TBAIan Crossfield

Past Colloquia
DateTalk TitleSpeaker
March 13, 2019
Astronomy Colloquium
Simulating Galaxy Formation: Illustris, IllustrisTNG and BeyondMark Vogelsberger, MIT
March 6, 2019
KICP Colloquium
Direct Detection of sub-GeV Dark Matter: A New FrontierRouven Essig, Stony Brook University
February 27, 2019
Astronomy Colloquium
The Dynamic Infrared SkyMansi Kasliwal, Caltech
February 20, 2019
KICP Colloquium
Constraints on Quantum GravityHirosi Ooguri, Caltech & Kavli IPMU
February 13, 2019
Astronomy Colloquium
Extreme AstrophysicsRoger Blandford, Stanford University
February 6, 2019
KICP Colloquium
The Planck last releaseJean-Loup Puget, IAS Université Paris-sud
January 30, 2019 cancelled
Astronomy Colloquium
Infrared Spectroscopy of Stars and PlanetsIan Crossfield, MIT
January 23, 2019
KICP Colloquium
A New Frontier in the Search for Dark MatterGordan Krnjaic, Fermilab
January 16, 2019
Astronomy Colloquium
Cosmic ReionizationNick Gnedin, University of Chicago/Fermilab
January 9, 2019
KICP Colloquium
How many numbers does it take to determine our Universe?Michael Turner, KICP

How many numbers does it take to determine our Universe?
January 9, 2019 | ERC 161 | 3:30 PM | KICP Colloquium
Click on the image to enlarge
Michael Turner, KICP

Since 2013, the Planck Surveyor team has made a good case that it takes six numbers to describe the whole Universe (fewer than the ten digits in a phone number), based upon their all-sky map of the CMB. Others have different opinions: zero, one, two, six (a different), and nine to describe our Universe. As I will discuss, the choice of numbers reveals much about what we know and our aspirations, as well as how we think about the Universe. After exploring the landscape, I will advocate for zero numbers and discuss the path and strategy to get there.

Cosmic Reionization
January 16, 2019 | ERC 161 | 3:30 PM | Host: Hsiao-Wen Chen | Astronomy Colloquium
Click on the image to enlarge
Nick Gnedin, University of Chicago/Fermilab

Cosmic reionization - ionization of the bulk of cosmic gas by ultraviolet radiation from first galaxies and quasars - is the least explored epoch in cosmic history. While significant progress has been made recently with the HST Frontier Fields program, the major breakthrough is still in the future, but not a distant one. The launch of JWST will start a revolution in studies of cosmic reionization, and other advanced observational probes will follow soon.

As observers are preparing for the flood of new data, theorists are currently busy revamping their tools to stay on par with future observations. This fortunate match between theory and observations will lead to a major breakthrough in this last cosmic frontier.

A New Frontier in the Search for Dark Matter
January 23, 2019 | ERC 161 | 3:30 PM | KICP Colloquium
Gordan Krnjaic, Fermilab

The gravitational evidence for the existence of dark matter is overwhelming; observations of galactic rotation curves, the CMB power spectrum, and light element abundances independently suggest that over 80% of all matter is "dark" and beyond the scope of the Standard Model. However, its particle nature is currently unknown, so discovering its potential non-gravitational interactions is a major priority in fundamental physics. In this talk, I will survey the landscape of light dark matter theories and and introduce an emerging field of fixed-target experiments that are poised to cover hitherto unexplored dark matter candidates with MeV-GeV masses. These new techniques involve direct dark matter production with proton, electron, and *muon* beams at various facilities including Fermilab, CERN, SLAC, and JLab. Exploring this mass range is essential for fully testing a broad, predictive class of theories in which dark matter abundance arises from dark-visible interactions in thermal equilibrium in the early universe.

Infrared Spectroscopy of Stars and Planets
January 30, 2019 cancelled | ERC 161 | 3:30 PM | Host: Jacob L. Bean | Astronomy Colloquium
Click on the image to enlarge
Ian Crossfield, MIT


Extrasolar planets and cool stars emit most of their light beyond the range of standard optical observations. These objects are often best studied using infrared spectroscopy. I will present recent results from my group on two topics: space-based IR spectroscopy of exoplanet atmospheres, and ground-based, high-resolution spectroscopy of both planets and stars. I will also conclude with a brief discussing of how future IR-optimized observatories will also enable exciting new science in these areas.

The Planck last release
February 6, 2019 | ERC 161 | 3:30 PM | KICP Colloquium
Jean-Loup Puget, IAS Université Paris-sud

The Planck High frequency maps improvements will be described together with some of their associated cosmology results. Implications for future experiments will also be discussed.

Extreme Astrophysics
February 13, 2019 | ERC 161 | 3:30 PM | Astronomy Colloquium
Roger Blandford, Stanford University

The electromagnetic spectrum has been opened up from meter radio waves to 100 TeV photons and augmented with 10 - 300 Hz gravitational wave, MeV - PeV neutrinos and MeV - ZeV (160 Joule) cosmic ray messages. Consequently, there is a high rate of discovery and understanding of phenomena whose explanation invokes accepted physics - classical (including general relativity), atomic, nuclear and particle (including QED) processes - in extreme environments. The richness of the discovery space can be epitomized by describing some new observations and ideas pertaining to relativistic jets formed by massive spinning black holes, Ultra High Energy Cosmic Rays accelerated by strong shock waves surrounding rich clusters of galaxies and Fast Radio Bursts, generated by neutron stars with 100 GT magnetic fields.

Constraints on Quantum Gravity
February 20, 2019 | ERC 161 | 3:30 PM | KICP Colloquium
Hirosi Ooguri, Caltech & Kavli IPMU

Superstring theory is our best candidate for the ultimate unification of general relativity and quantum mechanics. Although predictions of the theory are typically at extremely high energy and out of reach of current experiments and observations, several non-trivial constraints on its low energy effective theory have been found. Because of the unusual ultraviolet behavior of gravitational theory, the standard argument for separation of scales may not work for gravity, leading to robust low energy predictions of consistency requirements at high energy. In this colloquium talk, I will start by explaining why the unification of general relativity and quantum mechanics has been difficult. After introducing the holographic principle as our guide to the unification, I will discuss its use in finding constraints on symmetry in quantum gravity. I will also discuss other conjectures on low energy effective theories, collectively called swampland conditions, with various levels of rigors. They include the weak gravity conjecture, which gives a lower bound on Coulomb-type forces relative to the gravitational force, and the distance conjecture, which is about structure of the space of scalar fields. I will discuss consequences of the conjectures.

The Dynamic Infrared Sky
February 27, 2019 | ERC 161 | 3:30 PM | Astronomy Colloquium
Click on the image to enlarge
Mansi Kasliwal, Caltech

The dynamic infrared sky is hitherto largely unexplored. The infrared is key to understand elusive stellar fates that are opaque, cold or dusty. The infrared unveiled the otherwise opaque heavy element nucleosynthesis in neutron star mergers. I will describe multiple projects to chart the time-domain in the infrared. I will begin with the SPitzer InfraRed Intensive Transients Survey (SPIRITS) −−− a systematic search of 194 nearby galaxies within 30 Mpc, on timescales ranging between a week to a year, to a depth of 20 mag with Spitzer's IRAC camera. SPIRITS has already uncovered over 131 explosive transients and over 2536 strong variables. Of these, 64 infrared transients are especially interesting as they have no optical counterparts whatsoever even with deep limits from Keck and HST. Interpretation of these new discoveries may include (i) deeply enshrouded supernovae, (ii) stellar mergers with dusty winds, (iii) 8--10 solar mass stars experiencing e-capture induced collapse in their cores, (iv) the birth of massive binaries that drive shocks in their molecular cloud, or (v) formation of stellar mass black holes. Motivated by the treasure trove of SPIRITS discoveries, we just commissioned Palomar Gattini-IR - a new 25 sq deg J-band camera to robotically chart the dynamic infrared sky. We have also begun building WINTER - a new 1 sq deg yJH-band camera on a new 1m telescope at Palomar Observatory.

Direct Detection of sub-GeV Dark Matter: A New Frontier
March 6, 2019 | ERC 161 | 3:30 PM | KICP Colloquium
Click on the image to enlarge
Rouven Essig, Stony Brook University

Dark matter makes up 85% of the matter in our Universe, but we have yet to learn its identity. While most experimental searches focus on Weakly Interacting Massive Particles (WIMPs) with masses above the proton (about 1 GeV/c^2), the theoretical landscape of possible dark-matter candidates has expanded significantly over the last decade, to consider masses from 10^-22 eV/c^2 up to the Planck mass, and even higher in the case of composite dark matter. A broad search program is therefore needed to maximize our chances of identifying dark matter. In this talk, I will discuss the search for dark matter with masses between about 500 keV/c^2 to 1 GeV/c^2, which has seen tremendous progress in the last few years. I will describe several direct-detection strategies that can probe this under-explored mass range, including searching for dark matter interactions with electrons in noble liquids, semiconductors, and scintillators, as well as searching for interactions with molecules to excite vibrational states. I will in particular highlight SENSEI, a funded experiment that will use new ultra-low-threshold silicon CCD detectors ("Skipper CCDs"). I will describe the first results from SENSEI and show how SENSEI, and the upcoming DAMIC-M, will probe vast new regions of parameter space in the next few years. I will also mention how placing a Skipper CCD on a satellite could probe strongly interacting sub-GeV dark matter.

Simulating Galaxy Formation: Illustris, IllustrisTNG and Beyond
March 13, 2019 | ERC 161 | 3:30 PM | Astronomy Colloquium
Click on the image to enlarge
Mark Vogelsberger, MIT

Cosmological simulations of galaxy formation have evolved significantly over the last years. In my talk, I will describe recent efforts to model the large-scale distribution of galaxies with cosmological hydrodynamics simulations. I will focus on the Illustris simulation, and our new simulation campaign, the IllustrisTNG project. After demonstrating the success of these simulations in terms of reproducing an enormous amount of observational data, I will also talk about their limitations and directions for further improvements over the next couple of years.

Why doesn't the Solar System have close-in super-Earths?
April 3, 2019 | ERC 161 | 3:30 PM | Host: Jacob L. Bean | Astronomy Colloquium
Sean Raymond, Laboratoire d'Astrophysique de Bordeaux, France

Jupiter is the only planet in our system that would be detectable if the Sun were observed from afar with current instruments. Its wide, near-circular orbit makes it a ~10% rarity among known giant exoplanets and the Solar System a ~1% rarity among Sun-like stars. Another oddity of the Solar System is the absence of close-in super-Earths, which are found around a significant fraction (~50%) of main sequence stars.

Models for the origin of close-in super-Earths can match the distributions of observed systems, although the compositions of super-Earths (icy vs rocky) are a key constraint. However, models are generally too efficient, and cannot explain systems like ours without super-Earths. Jupiter's
growth may provide an answer. If Jupiter's core formed quickly, it would have blocked the flux of small `pebbles' drifting inward through the disk and starved the terrestrial planets' building blocks. Once Jupiter was fully-grown it opened a gap in the Sun's protoplanetary disk and may have
blocked the inward migration of larger cores, protecting the inner Solar System from icy invaders than instead formed the ice giants and Saturn's core. These ideas remain incomplete but have the promise to explain how the Solar System fits in the larger context.

Refreshments served at 4:30 PM, Hubble Lounge

The Search for Biosignature Gases on Exoplanets
April 10, 2019 | ERC 161 | 3:30 PM | Host: John E. Carlstrom | Astronomy Colloquium
Sara Seager, MIT

Thousands of exoplanets are known to orbit nearby stars and small rocky planets are established to be common. The ambitious goal of identifying a habitable or inhabited world is within reach. But how likely are we to succeed? We need to first discover a pool of planets in their host star's "extended" habitable zone and second observe their atmospheres in detail to identify the presence of water vapor, a requirement for all life as we know it. Life must not only exist on one of those planets, but the life must produce "biosignature gases" that are spectroscopically active, and we need to be able to sort through a growing list of false-positive scenarios with what is likely to be limited data. The race to find habitable exoplanets has accelerated with the realization that "big Earths" transiting small stars can be both discovered and characterized with current technology, such that the James Webb Space Telescope has a chance to be the first to provide evidence of biosignature gases. Transiting exoplanets require a fortuitous alignment and the fast-track approach is therefore only the first step in a long journey. The next step is sophisticated starlight suppression techniques for large ground-and space-based based telescopes to observe small exoplanets directly. These ideas will lead us down a path to where future generations will implement very large space-based telescopes to search thousands of all types of stars for hundreds of Earths to find signs of life amidst a yet unknown range of planetary environments. What will it take to identify such habitable worlds with the observations and theoretical tools available to us?

Refreshments served at 4:30 PM, Hubble Lounge

May 1, 2019 | ERC 161 | 3:30 PM | Host: Craig J. Hogan | Astronomy Colloquium
Dara Norman

Refreshments served at 4:30 PM, Hubble Lounge

May 15, 2019 | ERC 161 | 3:30 PM | Host: Hsiao-Wen Chen | Astronomy Colloquium
Rob Kennicutt

Refreshments served at 4:30 PM, Hubble Lounge

May 29, 2019 | ERC 161 | 3:30 PM | Host: Hsiao-Wen Chen | Astronomy Colloquium
Ian Crossfield

Refreshments served at 4:30 PM, Hubble Lounge