March 2014

DATE EVENT LOCATION
Tuesday, Mar 4
3:45 pm — 4:45 pm
LPL Colloquium: Dr. John Grotzinger
Dr. John Grotzinger
Fletcher Jones Professor of Geology
California Institute of Technology
Overview of MSL results
Kuiper Space Sciences: Room 312
Monday, Mar 10
4:00 pm — 5:00 pm
TAP Colloquium: Shunsaku Horiuchi
Shunsaku Horiuchi
University of California, Irvine

Neutrino probes of Cosmic Explosions
The collapse of massive stars and their subsequent explosions are among the most energetic phenomena in the Universe and impact many topics in astrophysics, from the chemical enrichment of galaxies to the generation of cosmic rays. Physically, all four fundamental forces of nature play important roles in shaping the core collapse, and the complexity has meant a complete understand of how the collapse reverses to drive an explosion eludes us to this day. On the other hand, the same complex richness makes the core collapse an inherently multi-messenger phenomenon. I will introduce current and upcoming neutrino and multi-messenger probes and discuss how they allow the study of the explosion's interiors and offer new insights into the core collapse and outcomes. In the process, I will highlight the interplay of astrophysics and particle physics. Multi-messenger astronomy is well-positioned to become a new window in which to study the Universe, promising to bring new insights - and potentially surprises.
Host: Shufang Su

Physics: Room 218
Tuesday, Mar 11
3:45 pm
LPL Graduate Student Colloquium: Thaddeus Komacek and Molly Simon
Thaddeus Komacek
Graduate Student in the Department of Planetary Sciences

Review of: "Ohmic Dissipation in the Interiors of Hot Jupiters"
X. Huang and A. Cumming, 2012, Astrophysical Journal, 757


Molly Simon
Graduate Student in the Department of Planetary Sciences

Review of: "Forming Circumbinary Planets: N-Body Simulations of Kepler-34"
S. Lines et al. 2014, Astrophysical Journal (in press)
Kuiper Space Sciences: Room 312
Tuesday, Mar 11
4:00 pm
Blitzer Award Lecture: Kenneth A. Johns, Ph.D.
The Professor Leon and Pauline Blitzer Award for Excellence in the Teaching of Physics and Related Sciences

Awardee and Speaker
Kenneth A. Johns, Ph.D.
Professor and Associate Head with the Department of Physics

The Higgs Boson and Beyond

Reception to follow in the Steward Observatory Lobby.
Steward Observatory: Room N210
Saturday, Mar 15–Sunday, Mar 23
Spring recess:
Saturday, Mar 15–Sunday, Mar 16
9:30 am — 5:30 pm
Tucson Festival of Books:
Tucson Festival of Books
LPL is at the Tucson Festival of Books this weekend! We'll be located in Science City. Come check us out!

LPL is also pleased to host the book launch event for "Orbiting Ray Bradbury's Mars," Saturday, March 15, 2:00p.m., Kuiper 308, featuring key note speaker Dr. Peter Smith, LPL Professor Emeritus.
UA Mall: Room
Saturday, Mar 15
2:00 pm
Book Launch: Orbiting Ray Bradbury's Mars
Orbiting Ray Bradbury's Mars
Edited by Gloria McMillan
Where else can you meet live Martian tour guides to the many dimensions of Ray Bradbury than at this festive book launch? Join us to celebrate a special collection of essays by NASA scientists, film experts, and literary writers.
Keynote speaker: Professor Emeritus Peter Smith

Mars Madness at the University of Arizona Libraries
Kuiper Space Sciences: Room 308
Monday, Mar 17–Friday, Mar 21
45th LPSC :
45th Lunar and Planetary Science Conference
Tuesday, Mar 18
7:30 pm
Steward Observatory Evening Lecture: Dr. Jill Tarter
Dr. Jill Tarter
Bernard M. Oliver Chair, SETI Institute

The Cosmos and You: Why Investing In The Search for Intelligent Life Beyond Earth Is Important To Long Future Of Humanity
The story of humanity began billions of years ago; you are intimately connected to the cosmos that made you. The only near term method of discovering whether we Earthlings can outgrow our technological adolescence and enjoy a long future is to determine the average longevity of technological civilizations in the Milky Way Galaxy. Today, we do not know whether there are any other technological civilizations; we could be unique. In physics we count 1,2, ∞ when only one example of a phenomenon is known, it could be singular, but as soon as a second example is found, we know there are many. N=2 is the important number for SETI. There are many indicators and futurists that suggest this could well be our last century as a technological civilization, but the successful detection of evidence of another technological civilization would mean that someone else has survived into old age, and therefore could provide abundant motivation for us to do so ourselves.
Social Science Bldg.: Room 100
Thursday, Mar 27
3:45 pm
LPL Colloquium: Dr. Youssef Moudden
Dr. Youssef Moudden
Research Associate
University of Colorado, Boulder

Challenges of simulating the martian atmosphere
Abstract:
Numerical modeling of planetary atmospheres has long been a prominent
tool for planetary exploration as well as the corner stone of all
weather prediction and climate studies on Earth. The most comprehensive
atmospheric numerical models are called General Circulation Models,
and they tend to incorporate a numerical representation of the most
important processes occurring in a planetary atmosphere. Each planet has
its unique characteristics and challenges when it comes to building
a GCM for its atmosphere. This presentation will list the particularities
and challenges of simulating the martian atmosphere.
Host: Roger Yelle
Kuiper Space Sciences: Room 312
Friday, Mar 28
12:00 pm — 1:00 pm
Brown Bag Colloquium: Dr. Youssef Moudden
Dr. Youssef Moudden
Research Associate
University of Colorado, Boulder

Data assimilation applied to planetary atmospheres
Abstract:
Data assimilation in atmospheric science refers to the process through
which systematic observations of different nature and sources are combined
with a numerical model to produce a more accurate simulation. Data
assimilation has been the key that enabled weather forecasting on Earth
and is extensively used for climate studies. Only recently has this
technique been attempted for Mars and contemplated for other planets.
This presentation will explain the workings of Data Assimilation and the
benefits that can be reaped from its application to other planets.
Kuiper Space Sciences: Room 309
Saturday, Mar 29
12:00 pm
Flandrau Planetarium: Girls Need Their Space
Girls Need Their Space
Hey Girls! Love stargazing? Want to learn more about the universe through hands-on experiments? Interested in learning what it's like to be a scientist from women behind some amazing discoveries in planetary science and astronomy? Come to Girls Need Their Space!

Indoor Activities start at noon - 6:00 pm.
Laser Show @ 6:00 pm.
Outdoor Star Party starts 7:00 - 9:00 pm.

For more information go to Girls Need Their Space.
Flandrau Planetarium: Room
Monday, Mar 31
4:00 pm — 5:00 pm
TAP Colloquium: Jennifer Siegel-Gaskins
Jennifer Siegel-Gaskins
California Institute of Technology

Dark matter signals from the Inner Galaxy?
Dark matter makes up roughly 80% of the matter in the universe, yet the details of its particle nature remain unknown. Many particle dark matter candidates can pair annihilate or decay to produce Standard Model particles, including gamma rays, charged particles, and neutrinos. The detection of these indirect signals of the annihilation or decay of dark matter in our Galaxy and beyond is a promising method for identifying dark matter, understanding its intrinsic properties, and mapping its distribution in the universe. Recent indirect searches with gamma rays have yielded several tantalizing hints of dark matter signals from the Inner Galaxy, however a confident detection remains elusive. I will discuss these recent results and possible alternatives to the dark matter interpretation of the claimed signals, as well as new approaches and prospects for robustly identifying a dark matter signal from the Inner Galaxy with upcoming experiments.

Host: Ina Sarcevic
TAP Colloquia
Physics: Room 224