Akshata Krishnamurthy

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Akshata Krishnamurthy
DrAkshataKrishnamurthy-1.jpg
Born (1990-12-27) December 27, 1990 (age 33)
Citizenship Indian
Alma mater Massachusetts Institute of Technology Ph.D.
OccupationsEngineering career
Discipline Space Systems
Employer(s) NASA Jet Propulsion Laboratory
Projects Mars 2020
NISAR
TESS
ASTERIA
Awards

Akshata Krishnamurthy (Born December 27, 1990) is an Indian space systems engineer working as Principal Investigator and Science Phase Lead at the NASA Jet Propulsion Laboratory. [1] [2]

Contents

She is currently working on Mars 2020. [3] She was named to Fortune India's "Most Powerful Women" [4]

Education

Krishnamurthy was born in Bengaluru, Karnataka, India, on December 27th, 1990, and completed her schooling and undergraduate education at 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. [5]

Krishnamurthy earned her PhD in Aeronautics and Astronautics from the Massachusetts Institute of Technology (MIT). [6] [7] Her PhD research focused on instrument calibration and performance improvement for space-based telescope missions for exoplanet detection. The results of her research contributed to the Transiting Exoplanet Survey Satellite (TESS) and Arcsecond Space Telescope Enabling Research in Astrophysics (ASTERIA) missions. Krishnamurthy and her colleagues contributed to the discovery of several exoplanets and the characterization of HD 59640 as an eruptive variable star with flares. [8] Other projects included the Mars 2020 Mars Oxygen ISRU Experiment (MOXIE). [9]

At MIT, she was the President of the Graduate Association of Aeronautics and Astronautics (GA^3) student organization [10] and Co-Chair of the MIT India Conference. [11]

Career

Krishnamurthy interned at NASA's Jet Propulsion Laboratory as part of the ASTERIA mission while working on her PhD. In April 2021, she and her colleagues received the NASA Group Achievement Award for their work with the CubeSat ASTERIA. [12] [13] Following graduation, she was employed as a systems engineer and science data system lead at the Jet Propulsion Laboratory. [14] She also started as a systems engineer on the NASA-ISRO Synthetic Aperture Radar (NISAR) mission [15] and later became the Science Phase Lead. [16]

Krishnamurthy is currently a robotic operations systems engineer working on the Mars 2020 Perseverance Mission robotic operations and a principal investigator on a strategic university research program with the Massachusetts Institute of Technology. [3] She previously served as an instrument engineer on NASA's Transiting Exoplanet Survey Satellite (TESS) and as a co-investigator on ASTERIA missions. She was noted as the first Indian to operate the Perseverance Mars rover. [17]

Awards and recognition

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References

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  2. "NASA JPL NISAR Project Team". NASA JPL. Retrieved 14 November 2024.
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  5. Krishnamurthy, Akshata (2012). Development and characterization of an inertial electrostatic confinement thruster (M.S. thesis). UIUC . Retrieved 21 December 2023.
  6. Krishnamurthy, Akshata (2020). Instrument systematics calibration and performance validation for high precision photometry missions (Ph.D. thesis). MIT. hdl:1721.1/128056 . Retrieved 21 December 2023.
  7. "Thesis Defense Presented by Akshata Krishnamurthy". MIT. 6 January 2020. Archived from the original on 26 September 2020.
  8. Günther, Maximilian N.; Zhan, Zhuchang; Seager, Sara; Rimmer, Paul B.; Ranjan, Sukrit; Stassun, Keivan G.; Oelkers, Ryan J.; Daylan, Tansu; Newton, Elisabeth; Kristiansen, Martti H.; Olah, Katalin; Gillen, Edward; Rappaport, Saul; Ricker, George R.; Vanderspek, Roland K. (20 January 2020). "Stellar Flares from the First TESS Data Release: Exploring a New Sample of M Dwarfs". The Astronomical Journal. 159 (2): 60. arXiv: 1901.00443 . Bibcode:2020AJ....159...60G. doi: 10.3847/1538-3881/ab5d3a . ISSN   0004-6256.
  9. Meyen, Forrest; Krishnamurthy, Akshata; Hoffman, Jeffrey (2018). "Mars 2020 MOXIE Publication". 2018 IEEE Aerospace Conference. doi:10.1109/AERO.2018.8396586. S2CID   49539396 . Retrieved 21 December 2023.
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