2034 Bernoulli (), provisional designation 1973 EE, is a stony asteroid from the inner regions of the asteroid belt, approximately 9 kilometers in diameter.
The asteroid was discovered on 5 March 1973, by Swiss astronomer
Paul Wild at Zimmerwald Observatory near Bern, Switzerland, and named for the members of the Bernoulli family. 
Orbit and classification
Bernoulli orbits the Sun in the inner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,230 days). Its orbit has an eccentricity of 0.18 and an inclination of 9 ° with respect to the ecliptic. The first used  precovery was taken at Palomar Observatory in 1951, extending the asteroid's observation arc by 22 years prior to its official discovery, while the first unused observation was made ten years earlier at Uccle Observatory in 1941.
Bernoulli is an assumed, common, stony S-type asteroid.
lightcurve of Bernoulli was obtained from photometric observations by Michael Alkema at the U.S. Elephant Head Observatory ( ), Arizona, in December 2012. Lightcurve analysis gave a G35 rotation period of hours with a brightness variation of 0.21 6.248 magnitude ( ). U=2+
Diameter and albedo
According to the survey carried out by the
NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, Bernoulli measures 7.8 and 8.5 kilometers in diameter and its surface has an albedo of 0.17 and 0.22, respectively,  while the  Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 9.4 kilometers with an absolute magnitude of 12.5.
minor planet was named in honour of the Bernoulli family, a dynasty of mathematicians from the city of Basel, Switzerland. In particular, Jacob Bernoulli (1654–1705), founder of the calculus of variations, Daniel Bernoulli (1700–1782), co-founder of hydrodynamics, and Johann Bernoulli (1667–1748), contributor to integral calculus and the teacher of Leonhard Euler, after whom the minor planet 2002 Euler is named.
The lunar crater
also honors the Swiss dynasty. Bernoulli The official naming citation was published by the  Minor Planet Center on 1 June 1980 ( ). M.P.C. 5359
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"JPL Small-Body Database Browser: 2034 Bernoulli (1973 EE)" (2017-05-05 last obs.). Jet Propulsion Laboratory . Retrieved . 10 June 2017
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Schmadel, Lutz D. (2007). "(2034) Bernoulli". Dictionary of Minor Planet Names – (2034) Bernoulli. Springer Berlin Heidelberg. p. 165. doi: 10.1007/978-3-540-29925-7_2035. ISBN . 978-3-540-00238-3
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"LCDB Data for (2034) Bernoulli". Asteroid Lightcurve Database (LCDB) . Retrieved . 16 May 2016
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Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv: . 1406.6645 Bibcode: 2014ApJ...791..121M. doi: 10.1088/0004-637X/791/2/121 . Retrieved . 8 December 2016
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Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: . 1109.6407 Bibcode: 2011ApJ...741...90M. doi: 10.1088/0004-637X/741/2/90 . Retrieved . 16 May 2016
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Alkema, Michael S. (July 2013). "Asteroid Lightcurve Analysis at Elephant Head Observatory: 2012 November - 2013 April". The Minor Planet Bulletin. 40 (3): 133–137. Bibcode: 2013MPBu...40..133A. ISSN 1052-8091 . Retrieved . 1 November 2015
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"2034 Bernoulli (1973 EE)". Minor Planet Center . Retrieved . 16 May 2016
"MPC/MPO/MPS Archive". Minor Planet Center . Retrieved . 16 May 2016