Film & Animation

The Hubble Space Telescope: From Cosmological Conflict to Alien Atmospheres

Tom Brown, Space Telescope Science Institute

The Hubble Space Telescope is one of the most successful scientific experiments in history: It maps the accelerating expansion of the cosmos, explores distant galaxies in the early universe, reveals the birth of stellar systems, and probes planets orbiting our sun and other stars. As one of the largest telescopes ever launched into orbit, Hubble’s unique capabilities drive diverse discoveries across all of astrophysics and extend the work of other observatories on the ground and in space. Join Dr. Brown as he highlights some of Hubble’s most exciting results and our expectations for the coming decade.

Host: Frank Summers, Space Telescope Science Institute
Recorded live on Tuesday, March 2, 2021.
More information: www.stsci.edu/public-lectures

The Milky Way vs. Andromeda: When Galaxies Collide

Laura Prichard, Space Telescope Science Institute

Our sun is one of hundreds of billions of stars that make up the spiral disk of our Milky Way galaxy. In turn, our galaxy is one of a hundred billion more that we can observe in the universe.

Join Dr. Prichard as she delves into the discovery of these “island universes” and explains how many types of galaxies form.

Take a tour of our galaxy’s neighborhood, including an adventure into our prospects of interstellar travel. The exploration will reveal the ultimate fate of the Milky Way when it collides with our massive spiral neighbor, the Andromeda galaxy, in 4 billion years.

Host: Frank Summers, Space Telescope Science Institute
Recorded live on Tuesday, February 2, 2021
More information: www.stsci.edu/public-lectures

The Darkest Secrets of the Universe

Raja GuhaThakurta, University of California–Santa Cruz

The cosmos contains many mysteries that intrigue even the most experienced researchers. The interplay between known and unknown constantly shifts and aligns. For example, there lies a hidden connection between dark matter, the Periodic Table of elements, cosmic inflation, and Schrödinger’s Cat. Other confounding conundrums include galaxy cannibalism, black holes, gravitational lensing, and gravitational waves. Join Dr. GuhaThakurta as these dark secrets of the universe are revealed and explored.

Host: Frank Summers, Space Telescope Science Institute
Recorded live on Tuesday, January 19, 2021.
More information: www.stsci.edu/public-lectures

Ultra Deep Field: Looking Out into Space, Looking Back into Time

This six-minute visual exploration of the Hubble Ultra Deep Field showcases the characteristics and contents of this landmark observation, as well as its four-dimensional nature across both space and time. In particular, galaxies are seen to more than 12 billion light-years away / 12 billion years ago, allowing astronomers to trace the development of galaxies across cosmic time.

A deep field is a long exposure on a small field of view to observe the faintest objects possible. The Ultra Deep Field (UDF) represents the deepest visible light observation of the universe (deeper views are extensions / subsets of this 2004 image). Containing about 10,000 sources, the UDF provides a statistical sample of galaxies across the universe.

In this sequence, the three-dimensional model of the UDF data set uses NASA and other images and source catalogs. More than 5000 galaxies with cross-matched image cutout and distance measure are placed in their correct relative position throughout the long thin pyramid of the observation. To keep the fly-throughs succinct, the depth of the pyramid is shortened by a factor of a few hundred.

The visualization encompasses a suite of UDF science points in a single camera shot journey. Zooms, fades, fly-throughs, and overlay graphics visually express and highlight aspects such as the field of view, long exposure time, variety of galaxies, and extent across the observable universe. The critical idea that “looking farther out into space is also looking farther back in time” leads to examples, drawn directly from the data, of galaxy structure changing and growing over time.

The Ultra Deep Field and other deep field studies help astronomers study the distribution, characteristics, and development of galaxies across space and time.

Visualization: Frank Summers, Alyssa Pagan, Leah Hustak, Greg Bacon, Zolt Levay, Lisa Frattare (STScI)
Data: Anton Koekemoer, Bahram Mobasher, and HUDF Team
Music: “Autumn: Meditativo” by Dee Yan-Key CC BY-NC-SA 4.0

This presentation is based on work performed as part of the NASA’s Universe of Learning project and is supported by NASA under cooperative agreement award number NNX16AC65A. The NASA’s Universe of Learning (NASA’s UoL) project creates and delivers science-driven, audience-driven resources and experiences designed to engage and immerse learners of all ages and backgrounds in exploring the universe for themselves. The competitively-selected project represents a unique partnership between the Space Telescope Science Institute, Caltech/IPAC, NASA Jet Propulsion Laboratory, Center for Astrophysics | Harvard & Smithsonian, and Sonoma State University, and is part of the NASA Science Mission Directorate Science Activation program.

Shaping Galaxies with Supermassive Black Hole Winds

Dr. Mitchell Revalski, Space Telescope Science Institute

Galaxies are a diverse population with a wide range of sizes, shapes, intensity of star formation, and masses of the supermassive black holes at their cores. These seemingly distinct characteristics can show intriguing correlations. A key ingredient in forming those relationships may be supermassive black hole winds, which are energetic flows of gas powered by the light emitted from growing black holes. These winds can sculpt the shapes of galaxies, determine the rate at which stars are able to form, and push heavy elements into the voids between galaxies. Join us for a visual exploration of what recent observations and simulations have taught us about these winds and how they may influence the development of galaxies.

Host: Frank Summers, Space Telescope Science Institute
Recorded live on Tuesday, December 1, 2020
More information: www.stsci.edu/public-lectures

Fading Stingray Nebula

This video shows the drastic changes to the planetary nebula Hen 3-1357, nicknamed the Stingray nebula, over two decades as captured by NASA’s Hubble Space Telescope. The nebula is first seen as it was in 1996, with filaments and tendrils of gas glowing bright blue at its center. The wavy outer edges of gas also stand out against the dark background of the universe. The 1996 portrait then transitions to Hubble’s 2016 image, which shows a much dimmer nebula lacking in the pronounced wavy edges.
Credit: NASA, ESA, B. Balick (University of Washington), M. Guerrero (Instituto de Astrofísica de Andalucía), and G. Ramos-Larios (Universidad de Guadalajara), and J. DePasquale (STScI)