Sarah Ashley Ballard | |
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Born | 1984 (age 39–40) |
Education | B.A. Astrophysics, UC Berkeley Ph.D. Astronomy and Astrophysics, Harvard (2012) |
Known for | Discovery of Kepler-19c (first exoplanet by transit-timing variation) |
Scientific career | |
Fields | Exoplanetary astrophysics |
Thesis | In Pursuit of New Worlds: Searches for and Studies of Transiting Exoplanets from Three Space-Based Observatories (2012) |
Doctoral advisor | David Charbonneau |
Website | drballard |
Sarah Ballard (born 1984 [1] ) is an American astronomer who is a professor at the University of Florida. [2] She has been a Torres Fellow at the Massachusetts Institute of Technology, [3] [4] a L'Oreal Fellow, [5] and a NASA Carl Sagan Fellow. [6]
Ballard was part of a collaborative team that was the first to successfully use the transit-timing variation method. This resulted in her team's confirmation of this theoretical search procedure and the discovery of the Kepler-19 planetary system with that technique. [7] Ballard took part in the discovery of four exoplanets (early numbered) in the Kepler spacecraft mission prior to its finding of significant quantities of planets around other stars.
Ballard has spoken about her experience as a victim of sexual harassment, [8] [9] about imposter syndrome, and about the controversy over the proposed Thirty Meter Telescope at the Mauna Kea Observatories.
As an undergraduate, Ballard started out as a gender studies major at the University of California, Berkeley. [10] [11] She completed a bachelor's degree from Berkeley in astrophysics in 2007, with a minor in physics. [12] [ better source needed ] She did her graduate studies at Harvard University, completing a doctorate in astronomy and astrophysics in 2012 under the supervision of David Charbonneau. [12] [13]
Ballard was a NASA Carl Sagan Fellow at the University of Washington where she did postdoctoral work; [6] and in 2015 was awarded a Women in Science Fellows postdoctoral fellowship by L'Oréal USA to continue her research at MIT. [5]
Ballard took part in the discovery of four exoplanets before she turned 30 years old, including Kepler-19c, the first exoplanet found using the transit-timing variation method on data from the Kepler space telescope mission. [10] [14] [15]
Planet Discoveries of Sarah Ballard | |||||||||
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Planets Discovered: 4 | |||||||||
Number | Planet Designation | Type | Size Class | System | Constellation | Discoverer(s) | Year | Discovery Method | Telescope |
1 | Kepler-19b [15] | Exoplanet | Kepler-19 | Lyra | Sarah Ballard et al. | Transit | Kepler | ||
2 | Kepler-61b [15] | Exoplanet | Kepler-61 | Lyra | Sarah Ballard et al. | Transit | Kepler | ||
3 | Kepler-93b [15] | Exoplanet | Super-Earth [16] [17] | Kepler-93 | Lyra | Sarah Ballard et al. | Transit | Kepler | |
4 | Kepler-19c | Exoplanet | Kepler-19 | Lyra | Sarah Ballard et al. | 2011 | Transit-timing variation | Kepler | |
Table Legend: | |||||||||
Size class = Planet radius distribution (radius of Earth). [18] | Discovery method =
|
The transit-timing variation method (TTV) is one of two techniques, along with the transit-duration variation method, proposed in 2001 by astronomer Jordi Miralda-Escudé. [19] TTV was amplified upon in 2004 by astronomers Matthew J. Holman and Norman W. Murray; [20] and by Eric Agol, Jason Steffen, Re’em Sari, and Will Clarkson. [21] Ballard was the principal investigator in the 2009 application to use the Spitzer Space Telescope to examine "The First Exoplanet Smaller than the Earth". [22] Ballard led the team which precisely estimated the diameter of Kepler-93b to within 1 percent, using TTV. [16] [23]
When exoplanetologist Geoffrey Marcy resigned from the UC Berkeley faculty over charges that he had sexually harassed female undergraduate students, Ballard came out publicly as one of his victims in order to help bring attention to sexual harassment in academia. [24] [25] [26] In an interview published by Wired, she said that "In the parking lot outside her apartment [...] he gave her advice about her current relationship. She opened the door and stuck her legs out, eager to leave. [...] He put his hand on the back of her neck and told her to relax, that everything would work out with that boy". [27]
Ballard has written and conducted workshops on impostor syndrome. [28] [29] [30] [31] She was involved in a controversy about the proposed Thirty Meter Telescope at Mauna Kea Observatory. Her friend, Keolu Fox, a native Hawaiian, helped her see the issue from an indigenous perspective. [32] Ballard spoke about the issue despite fears about the effects it may have on her career. [32]
Ballard was one of a number of scientists who expressed concern in "An open letter to SCOTUS from professional physicists drafted by the Equity & Inclusion in Physics & Astronomy group" [33] following oral arguments in the U.S. Supreme Court case commonly known as Fisher II involving inclusiveness in admissions policies at the University of Texas.
In astronomy, a transit is the passage of a celestial body directly between a larger body and the observer. As viewed from a particular vantage point, the transiting body appears to move across the face of the larger body, covering a small portion of it.
These are lists of planets. A planet is a large, rounded astronomical body that is neither a star nor its remnant. The best available theory of planet formation is the nebular hypothesis, which posits that an interstellar cloud collapses out of a nebula to create a young protostar orbited by a protoplanetary disk. There are eight planets within the Solar System; planets outside of the solar system are also known as exoplanets.
Geoffrey William Marcy is an American astronomer. He was an early influence in the field of exoplanet detection, discovery, and characterization. Marcy was a professor of astronomy at the University of California, Berkeley, and an adjunct professor of physics and astronomy at San Francisco State University. Marcy and his research teams discovered many extrasolar planets, including 70 out of the first 100 known exoplanets and also the first planetary system around a Sun-like star, Upsilon Andromedae. Marcy was a co-investigator on the NASA Kepler space telescope mission. His collaborators have included R. Paul Butler, Debra Fischer and Steven S. Vogt, Jason Wright, Andrew Howard, Katie Peek, John Johnson, Erik Petigura, Lauren Weiss, Lea Hirsch and the Kepler Science Team. Following an investigation for sexual harassment in 2015, Marcy resigned his position at the University of California, Berkeley.
An exomoon or extrasolar moon is a natural satellite that orbits an exoplanet or other non-stellar extrasolar body.
Any planet is an extremely faint light source compared to its parent star. For example, a star like the Sun is about a billion times as bright as the reflected light from any of the planets orbiting it. In addition to the intrinsic difficulty of detecting such a faint light source, the light from the parent star causes a glare that washes it out. For those reasons, very few of the exoplanets reported as of January 2024 have been observed directly, with even fewer being resolved from their host star.
Kepler-4 is a sunlike star located about 1626 light-years away in the constellation Draco. It is in the field of view of the Kepler Mission, a NASA operation purposed with finding Earth-like planets. Kepler-4b, a Neptune-sized planet that orbits extremely close to its star, was discovered in its orbit and made public by the Kepler team on January 4, 2010. Kepler-4b was the first discovery by the Kepler satellite, and its confirmation helped to demonstrate the spacecraft's effectiveness.
Transit-timing variation is a method for detecting exoplanets by observing variations in the timing of a transit. This provides an extremely sensitive method capable of detecting additional planets in the system with masses potentially as small as that of Earth. In tightly packed planetary systems, the gravitational pull of the planets among themselves causes one planet to accelerate and another planet to decelerate along its orbit. The acceleration causes the orbital period of each planet to change. Detecting this effect by measuring the change is known as transit-timing variations. "Timing variation" asks whether the transit occurs with strict periodicity or if there's a variation.
An exoplanet is a planet located outside the Solar System. The first evidence of an exoplanet was noted as early as 1917, but was not recognized as such until 2016; no planet discovery has yet come from that evidence. What turned out to be the first detection of an exoplanet was published among a list of possible candidates in 1988, though not confirmed until 2003. The first confirmed detection came in 1992, with the discovery of terrestrial-mass planets orbiting the pulsar PSR B1257+12. The first confirmation of an exoplanet orbiting a main-sequence star was made in 1995, when a giant planet was found in a four-day orbit around the nearby star 51 Pegasi. Some exoplanets have been imaged directly by telescopes, but the vast majority have been detected through indirect methods, such as the transit method and the radial-velocity method. As of 24 July 2024, there are 7,026 confirmed exoplanets in 4,949 planetary systems, with 1007 systems having more than one planet. This is a list of the most notable discoveries.
The NASA Exoplanet Science Institute (NExScI) is part of the Infrared Processing and Analysis Center (IPAC) and is on the campus of the California Institute of Technology (Caltech) in Pasadena, CA. NExScI was formerly known as the Michelson Science Center and before that as the Interferometry Science Center. It was renamed NExScI in the Fall of 2008 to reflect NASA's growing interest in the search for planets outside of the Solar System, also known as exoplanets. The executive director of NExScI is Charles A. Beichman.
The NASA Exoplanet Archive is an online astronomical exoplanet catalog and data service that collects and serves public data that support the search for and characterization of extra-solar planets (exoplanets) and their host stars. It is part of the Infrared Processing and Analysis Center and is on the campus of the California Institute of Technology (Caltech) in Pasadena, CA. The archive is funded by NASA and was launched in early December 2011 by the NASA Exoplanet Science Institute as part of NASA's Exoplanet Exploration Program. In June 2019, the archive's collection of confirmed exoplanets surpassed 4,000.
John Asher Johnson is an American astrophysicist and professor of astronomy at Harvard. He is the first tenured African-American physical science professor in the history of the university. Johnson is well known for discovering three of the first known planets smaller than the Earth outside of the solar system, including the first Mars-sized exoplanet.
Lisa Kaltenegger is an Austrian astronomer specialising in the modeling and characterization of exoplanets and the search for life. On July 1, 2014, she was appointed Associate Professor of Astronomy at Cornell University. Previously, she held a joint position at the Max Planck Institute for Astronomy in Heidelberg where she was the Emmy Noether Research Group Leader for the "Super-Earths and Life" group, and at the Center for Astrophysics | Harvard & Smithsonian in Cambridge, MA. She was appointed Lecturer in 2008 at Harvard University and 2011 at University of Heidelberg.
Kepler-37, also known as UGA-1785, is a G-type main-sequence star located in the constellation Lyra 209 light-years from Earth. It is host to exoplanets Kepler-37b, Kepler-37c, Kepler-37d and possibly Kepler-37e, all of which orbit very close to it. Kepler-37 has a mass about 80.3 percent of the Sun's and a radius about 77 percent as large. It has a temperature similar to that of the Sun, but a bit cooler at 5,357 K. It has about half the metallicity of the Sun. With an age of roughly 6 billion years, it is slightly older than the Sun, but is still a main-sequence star. Until January 2015, Kepler-37 was the smallest star to be measured via asteroseismology.
Natalie M. Batalha is professor of Astronomy and Astrophysics at UC Santa Cruz. Previously she was a research astronomer in the Space Sciences Division of NASA Ames Research Center and held the position of Science Team Lead, Mission Scientist, and Project Scientist on the Kepler Mission, the first mission capable of finding Earth-size planets around other stars. Before moving to NASA, Batalha was a Professor of Physics and Astronomy at San Jose State University.
Kepler-438b is a confirmed near-Earth-sized exoplanet. It is likely rocky. It orbits on the inner edge of the habitable zone of a red dwarf, Kepler-438, about 472.9 light-years from Earth in the constellation Lyra. It receives 1.4 times our solar flux. The planet was discovered by NASA's Kepler spacecraft using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. NASA announced the confirmation of the exoplanet on 6 January 2015.
The Nexus for Exoplanet System Science (NExSS) initiative is a National Aeronautics and Space Administration (NASA) virtual institute designed to foster interdisciplinary collaboration in the search for life on exoplanets. Led by the Ames Research Center, the NASA Exoplanet Science Institute, and the Goddard Institute for Space Studies, NExSS will help organize the search for life on exoplanets from participating research teams and acquire new knowledge about exoplanets and extrasolar planetary systems.
Tabetha "Tabby" Suzanne Boyajian is an American astronomer and associate professor at Louisiana State University. She works in of stellar interferometry, stellar spectroscopy, exoplanet research, and high angular resolution astronomy, all particularly at optical and infrared wavelengths. Boyajian was the lead author of the September 2015 paper "Where's the Flux?", which investigated the highly unusual light curve of KIC 8462852; the star is colloquially known as Tabby's Star in her honor.
Stephen Kane is a full professor of astronomy and planetary astrophysics at the University of California, Riverside who specializes in exoplanetary science. His work covers a broad range of exoplanet detection methods, including the microlensing, transit, radial velocity, and imaging techniques. He is a leading expert on the topic of planetary habitability and the habitable zone of planetary systems. He has published hundreds of peer reviewed scientific papers and has discovered/co-discovered several hundred planets orbiting other stars. He is a prolific advocate of interdisciplinarity science and studying Venus as an exoplanet analog.
Jessie Christiansen is an Australian astrophysicist who is the Chief Scientist of the NASA Exoplanet Science Institute at the California Institute of Technology (Caltech). She won the 2018 NASA Exceptional Engineering Achievement Medal for her work on the Kepler planet sample.
Eric Agol is an American astronomer and astrophysicist who was awarded a Guggenheim Fellowship in 2017.
A team led by Sarah Ballard...
Ballard and her team have made a major scientific advance...