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On May 27, 2023, CIERA Research Assistant Professor Aaron Geller and former NSF Graduate Fellow Alex Gurvich were featured on the American Astronomical Society (AAS) Journal Author Series to showcase Firefly, their new browser-based interactive tool for visualizing 3D particle data sets. Geller and Gurvich were interviewed by the AAS’s Frank Timmes. Read the full news story

New research suggests that a lack of a stable asteroid belt around these common, small, and cool stars may make their exoplanets less habitable for life. This edition of SETI Live features a conversation with lead researcher Anna C. Childs to explore the implications of this research and the future of the search for alien

Firefly video visualization of data from the the European Space Agency’s (ESA) Gaia satellite. The full demo enables users to explore all 1.46 billion stars in the Gaia DR3 dataset in real time. Firefly is a browser-based interactive particle visualization app created by CIERA researchers Alex Gurvich and Aaron Geller, in a joint venture with

An international team of astronomers, including Northwestern University’s Farhad Yusef-Zadeh, has discovered one of the largest structures ever observed in the Milky Way. A newly spotted pair of radio-emitting bubbles reach hundreds of light-years tall, dwarfing all other structures in the central region of the galaxy.

APERTURE: A Precise Extremely large Reflective Telescope Using Reconfigurable Elements. This is the deployment concept which was produced during the NIAC Phase I feasibility study. APERTURE is a UV-Visible telescope with a 16-m diameter primary mirror. The primary is a flexible membrane coated with magnetic smart material. The shape of the reflector can be corrected

Northwestern Physics and Astronomy student Shi Ye presents a talk as part of the Northwestern Ready Set Go (RSG) program. The goals of the program are to increase awareness for the urgent need for excellent research communicators and to coach graduate and post doctoral researchers to improve their own presentation skills. The program focuses on three important

Binary+single encounter that leads to an exchange, followed by a second binary+single encounter that leads to a collision Within star clusters, close encounters between single and multiple stars can be frequent and may lead to the production of exotic stars like X-ray sources and blue stragglers. By using the small-N-body code FEWBODY and another visualization

Triple+binary encounter that leads to a collision Within star clusters, close encounters between single and multiple stars can be frequent and may lead to the production of exotic stars like X-ray sources and blue stragglers. By using the small-N-body code FEWBODY and another visualization software, a few visualizations of interesting stellar encounters were created. In

Binary + single encounter that leads to a collision Within star clusters, close encounters between single and multiple stars can be frequent and may lead to the production of exotic stars like X-ray sources and blue stragglers. By using the small-N-body code FEWBODY and another visualization software, a few visualizations of interesting stellar encounters were

Binary+single encounter that leads to an exchange Within star clusters, close encounters between single and multiple stars can be frequent and may lead to the production of exotic stars like X-ray sources and blue stragglers. By using the small-N-body code FEWBODY and another visualization software, a few visualizations of interesting stellar encounters were created. In

This movie, Life of the Pleiades, was generated from an interactive visualization that Aaron Geller developed with Mark SubbaRao using Uniview. The interactive version can be shown on a planetarium dome, or rendered into a movie (as shown here). A 3D version of this movie exists in the Space Visualization Lab at the Adler Planetarium.

This movie shows one of the possible evolutionary scenarios of a binary system. Binary systems are star systems comprising two stars orbiting around their common center of mass in a Keplerian orbit, which means that the two components are bound together by their mutual gravitational attraction. In this movie, the binary system consists of a

This is a movie of the evolving color-magnitude diagram from the N-body model of the old open cluster NGC 188. Binaries are plotted with blue points, and show the combined light of the unresolved system. Single stars are plotted in black points. The dynamical and stellar evolution calculations were performed using NBODY6, with some modifications