Akshata Krishnamurthy | |
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Born | |
Citizenship | Indian |
Alma mater | Massachusetts Institute of Technology Ph.D. |
Occupation(s) | Engineering career |
Discipline | Space Systems |
Employer(s) | NASA Jet Propulsion Laboratory |
Projects | Mars 2020 NISAR TESS ASTERIA |
Awards | Luigi G. Napolitano Award, Dr. Robbin Chapman Excellence Through Adversity Award, IAF Emerging Space Leader |
Akshata Krishnamurthy is a space systems engineer working as Science Phase Lead at the NASA Jet Propulsion Laboratory. Born in India, Krishnamurthy has worked on Mars 2020, NISAR, TESS and ASTERIA missions.
Krishnamurthy was born in Bengaluru, Karnataka, India, and completed her schooling and undergraduate education from R.V. College of Engineering before moving to the United States to pursue a Master's degree in Aerospace Engineering from the University of Illinois at Urbana-Champaign. [1]
Krishnamurthy earned her PhD in Aeronautics and Astronautics from the Massachusetts Institute of Technology (MIT). [2] [3] Her PhD research [4] focused on instrument calibration and performance improvement for space-based telescope missions for exoplanet detection, and was used in two space missions, Transiting Exoplanet Survey Satellite (TESS) and Arcsecond Space Telescope Enabling Research in Astrophysics (ASTERIA). Krishnamurthy and her colleagues discovered several exoplanets, and characterized HD 59640 to be an eruptive variable stars with flares. [5] Other projects included the Mars 2020 Mars Oxygen ISRU Experiment (MOXIE). [6]
At MIT, she was the President of the Graduate Association of Aeronautics and Astronautics (GA^3) student organization., [7] and Co-Chair of the MIT India Conference [8] [9]
Krishnamurthy interned at NASA's Jet Propulsion Laboratory as part of the ASTERIA mission while working on her PhD. Following graduation, Krishnamurthy got a full-time position as a systems engineer and science data system lead at the Jet Propulsion Laboratory. She started as systems engineer on the NASA-ISRO Synthetic Aperture Radar (NISAR) mission [10] and continued to become the Science Phase Lead leading planning, development and testing for nominal science operations. [11] Krishnamurthy is a Robotic Operations Systems Engineer working on the Mars 2020 Perseverance Mission Robotic Operations and Principal Investigator on a Strategic University Research Program with MIT. [12] Previously, Krishnamurthy served as Instrument Engineer on NASA's Transiting Exoplanet Survey Satellite (TESS) and as co-investigator on ASTERIA missions.ASTERIA is the smallest telescope to ever detect an exoplanet. [13] [14]
She motivates millions of young students all over the world by sharing her journey as an immigrant on a visa in the United States, on Instagram, and persevering in the face of obstacles to achieve her dreams of working on space projects at NASA. [27] Her goal is to inspire millions of people to dream big and live their best lives. [28]
55 Cancri e is an exoplanet orbiting a Sun-like host star, 55 Cancri A. The mass of the exoplanet is about eight Earth masses and its diameter is about twice that of the Earth. 55 Cancri e was discovered on 30 August 2004, thus making it the first super-Earth discovered around a main sequence star, predating Gliese 876 d by a year. It is the innermost planet in its planetary system, taking less than 18 hours to complete an orbit. However, until the 2010 observations and recalculations, this planet had been thought to take about 2.8 days to orbit the star.
Transiting Exoplanet Survey Satellite (TESS) is a space telescope for NASA's Explorer program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission. It was launched on 18 April 2018, atop a Falcon 9 launch vehicle and was placed into a highly elliptical 13.70-day orbit around the Earth. The first light image from TESS was taken on 7 August 2018, and released publicly on 17 September 2018.
Planet Hunters is a citizen science project to find exoplanets using human eyes. It does this by having users analyze data from the NASA Kepler space telescope and the NASA Transiting Exoplanet Survey Satellite. It was launched by a team led by Debra Fischer at Yale University, as part of the Zooniverse project.
TOI-677 b is a confirmed "warm" super-Jupiter exoplanet orbiting TOI-677, its host star, in the Ophiuchus constellation, about 466 ly (143 pc) away from Earth. The planet was discovered by NASA's Transiting Exoplanet Survey Satellite (TESS) using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Discovery of the exoplanet was announced on 13 November 2019.
TOI-700 is a red dwarf 101.4 light-years away from Earth located in the Dorado constellation that hosts TOI-700 d, the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).
TOI-700 d is a near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf TOI-700, the outermost planet within the system. It is located roughly 101.4 light-years (31.1 pc) away from Earth in the constellation of Dorado. The exoplanet is the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).
Planet Patrol is a NASA citizen science project available in Zooniverse and aimed at discovering new exoplanets with data from the TESS telescope.
LHS 1815 b is a thick disk exoplanet, discovered in 2020 by TESS. The planet is located outside the galactic plane.
TOI-640 b is an exoplanet that was suspected since 2019. It's discovery has been confirmed by the TESS team in January 2021. It is located 1115 light years away from Earth, orbiting a primary F-class star in a binary star system with red dwarf and has an orbital period of 5 days.
L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs, as measured by the Gaia spacecraft.
TOI-1452 b is a confirmed super-Earth exoplanet, possibly a water world, orbiting a red-dwarf star TOI-1452 about 100 light-years away in the Draco constellation. The exoplanet is about 70% larger in diameter than Earth, and roughly five times as massive.