Natalie Batalha
 Natalie Batalha | |
|---|---|
 | |
| Rayuwa | |
| Haihuwa | Kalifoniya, 14 Mayu 1966 (58 shekaru) |
| ƙasa | Tarayyar Amurka |
| Ƴan uwa | |
| Abokiyar zama |
Celso Batalha (en)  |
| Karatu | |
| Makaranta |
University of California, Berkeley (en) University of California, Santa Cruz (en) |
| Sana'a | |
| Sana'a |
physicist (en) , astrophysicist (en) , Ilimin Taurari da university teacher (en) |
| Employers |
National Aeronautics and Space Administration (en) San José State University (en) University of California, Santa Cruz (en) (15 Oktoba 2018 - |
| Mamba |
American Academy of Arts and Sciences (en) |
| IMDb | nm5275581 |
Sana'a
[gyara sashe | gyara masomin]
A cikin 1997,William Borucki ya ƙara Batalha zuwa ƙungiyar kimiyya kuma ta fara aiki akan ɗaukar hoto.Ta kasance tare da Ofishin Jakadancin Kepler tun ƙira da kuɗi,kuma a matsayin ɗaya daga cikin masu binciken Co-Bincike na asali ne ke da alhakin zaɓin taurari sama da 150,000 da na'urar hangen nesa ke sa ido.Yanzu tana aiki tare da membobin ƙungiyar a Cibiyar Bincike ta Ames don gano taurari masu dacewa daga bayanan aikin Kepler. Ta jagoranci binciken da ya samar da binciken a cikin 2011 na Kepler 10b, wanda shine farkon da aka tabbatar da dutsen duniya a wajen tsarin hasken rana .
A cikin Nuwamba 2017,Cibiyar Kimiyya ta Sararin Samaniya ta zaɓi shirye-shirye 13 don Kimiyyar Sakin Farko na Direkta(DD-ERS)akan na'urar hangen nesa ta James Webb. Daga cikin jimlar sa'o'i 460 na lura da aka ware,aikin Batalha,'Transiting Exoplanet Community Shirin Sakin Kimiyya na Farko',an ba shi awa 86.9; mafi girma na kowane shirin DD-ERS akan JWST. An ware waɗannan sa'o'in dubawa don amfani da su a cikin watanni biyar na farkon aikin na'urar hangen nesa.