The Center for Astrophysics | Harvard & Smithsonian
The Center for Astrophysics | Harvard & Smithsonian
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Howard A. Smith

Center for Astrophysics
Senior Astrophysicist & Lecturer
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Howard A. Smith
hsmith@cfa.harvard.edu

About

Howard Smith is a physicist, infrared astronomer, and a member of the Astronomy Department. His research emphasizes the origins of stars in the galaxy and other galaxies, Active Galactic Nuclei, and a wide range of other cosmic infrared sources from very nearby Near Earth Objects to cosmologically distant, high-z galaxies using both ground and space telescopes, and (in between) the SOFIA Airborne Observatory. He has been a Co-I on instruments on international spacecraft, the PI of many grants, and has supervised numerous postdocs and students from PhD candidates to undergraduates. He has over 400 publications, and in addition to research, he serves as a special consultant in the Director's Office. Before coming to CfA, he was Chair of Astronomy at the Smithsonian's National Air and Space Museum where he designed and funded the Department and managed its staff, who did research and also played an active role in gallery development, public education (winning DOE’s national award for Best Program), and in the production of three IMAX movies including the Academy Award Nominee, "Cosmic Voyage." He spent three years as a Visiting Scientist at NASA HQ in charge of grants and proposed small missions. He writes regularly about recent astronomical discoveries, and about science and religion, for popular outlets and gives frequent public lectures. He did his PhD thesis research with Charles Townes at UC Berkeley.

PhD from UCBerkeley; BA from MIT

Telescopes and Instruments

Magellan Telescopes

The twin Magellan Telescopes in Chile are each 6.5 meter optical telescopes. These telescopes are both equipped with instruments to take images and spectra of light from a wide variety of astronomical sources, including exoplanet systems, star-forming regions, supernova remnants, and interacting galaxies. The Magellan Telescopes — named Baade and Clay —  are hosted at the Las Campanas Observatory and are operated by a consortium of institutions, including the Center for Astrophysics | Harvard & Smithsonian, Carnegie Institution for Science, University of Arizona, the University of Michigan, and the Massachusetts Institute of Technology. In addition, CfA scientists and engineers provided a wide field f/5 focal system (including secondary mirror and corrective optics), and a powerful astronomical camera for use at the Clay telescope.

Visit the Magellan Telescopes Website
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Giant Magellan Telescope

Is Earth unique, or are there other planets with life in the Milky Way? To answer this question and many others, astronomers need larger and more sensitive observatories than anything we currently have. For that reason, the Center for Astrophysics | Harvard & Smithsonian is collaborating with a number of other institutions around the world to create the Giant Magellan Telescope (GMT), currently under construction in Chile. The GMT will consist of seven large mirrors acting in concert as one giant telescope 80 feet across. That large size provides an unprecedented view of the sky and the ability to detect the chemical composition of exoplanet atmospheres. Like NASA’s Hubble Space Telescope, the GMT will be a powerful tool across the field of astronomy, providing insights into the formation of planets, the structure of galaxies, and the evolution of the universe itself.

Visit the GMT Website
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MMT Observatory

The MMT Observatory is the premier visible-light and infrared telescope jointly managed by the Smithsonian Astrophysical Observatory, part of the Center for Astrophysics | Harvard & Smithsonian, and the University of Arizona. Located at the Fred Lawrence Whipple Observatory (FLWO) in southern Arizona, this 6.5-meter (21 foot) telescope is used to study objects across the field of astronomy, from the Solar System to distant galaxies. The MMT has provided a testbed for new telescope technologies developed by scientists and engineers at the CfA and the University of Arizona.

Visit the MMT Website
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Pan-STARRS-1 Science Consortium

Many objects in the sky don’t change or move visibly on human time scales. However, many others do, especially objects in the Solar System. The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) program is designed to monitor the sky for transient astronomical phenomena: everything from near-Earth asteroids to supernovas in far-off galaxies. The first phase of the program, Pan-STARRS1, used a 1.8-meter telescope on the summit of Haleakalā on the island of Maui in Hawaii. The Center for Astrophysics | Harvard & Smithsonian is part of the international Pan-STARRS1 Science consortium, along with the University of Hawaii and other institutions around the world. Pan-STARRS1 data revealed many asteroids, comets, and other previously-unknown moving or variable astronomical objects.

Visit the Pan-STARRS1 Science Consortium Website
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Spitzer Space Telescope

Infrared light is the key to studying a wide range of astronomical systems, including newborn stars and planets, dust in distant galaxies, and material swirling around black holes. The Spitzer Space Telescope was NASA’s orbiting infrared observatory, and part of NASA’s Great Observatories program, along with the Chandra X-ray Observatory and the Hubble Space Telescope. Scientists and engineers at the Center for Astrophysics | Harvard & Smithsonian led the design, testing, and construction of the Infrared Array Camera (IRAC). The Spitzer Space Telescope was launched in 2003 and retired in 2020.

Visit the Spitzer Space Telescope IRAC Page
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SPHEREx

Clues about the origin of the universe and of life are scattered across the sky. SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) is a NASA medium-class Explorer (MIDEx) designed to measure optical-to-infrared spectra of hundreds of millions of galaxies and millions of Milky Way stars. With its unprecedented galaxy catalog, SPHEREx will answer pressing questions about the history and origin of the universe. Its unique catalog of Milky Way stellar spectra will reveal the abundances of water and other molecules associated with life in the Milky Way in unprecedented detail. Researchers from the Center for Astrophysics | Harvard & Smithsonian, including Gary Melnick, Matthew Ashby, Joseph Hora, and Volker Tolls, are involved in the SPHEREx investigation seeking to understand the distribution of these molecules throughout the Galaxy so as to better answer complex questions about their origins. SPHEREx is scheduled for launch from Vandenburg AFB no earlier than February 2025.Visit the SPHEREx Website
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Submillimeter Wave Astronomy Satellite

NASA’s Submillimeter Wave Astronomy Satellite (SWAS) was a space observatory built to look for water and other molecules associated with life as we know it. During its seven years of operation, SWAS provided the first measure of the distribution of water in the Milky Way. Astronomers also used the observatory to make important discoveries about the interstellar clouds where new stars and planets are born, as well as observations of planets and comets within the Solar System. Center for Astrophysics | Harvard & Smithsonian scientists and engineers designed the telescope for SWAS, and the CfA hosted the operations center for the spacecraft. SWAS operated from 1998 through 2005, when it was put into hibernation mode.

Visit the SWAS Website
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SOFIA (Stratospheric Observatory for Infrared Astronomy)

Earth’s atmosphere protects us from harmful radiation, but it also blocks a lot of light useful for astronomy. For that reason, NASA and the German Aerospace Center (DLR) built the Stratospheric Observatory for Infrared Astronomy (SOFIA) to fly aboard a modified commercial aircraft capable of flying above 99% of the light-blocking atmosphere. SOFIA is a powerful, general-purpose infrared observatory used to study the birth of new stars, planetary nebulas and supernova remnants, the atmospheres of Solar System objects, and many more. The American portion of SOFIA management is handled by the Universities Space Research Association (USRA), a private educational corporation consisting of over 100 institutions, including the Center for Astrophysics | Harvard & Smithsonian.

Visit the SOFIA Website
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The Submillimeter Array - Maunakea, HI

Located near the summit of Maunakea on the Big Island of Hawaii, the Submillimeter Array (SMA) is one of the flagship observatories of the Center for Astrophysics | Harvard & Smithsonian. The observatory consists of eight radio dishes working together as one telescope, giving astronomers a window on a wide range of astronomical objects and phenomena: planets and comets in our own Solar System; the birth of stars and planets; and the supermassive black holes hidden at the centers of the Milky Way and other galaxies. The SMA is operated jointly by the CfA and the Academia Sinica in Taiwan.

Visit the Submillimeter Array Website
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