Ivano Bertini

Ivano Bertini (born April, 1968, in Milan, Italy) is an Italian astronomer at the University of Padua.[1]

Scientific career

Bertini got the Master degree in Astronomy at the University of Padua in 2001, discussing a thesis about the discovery, astrometry, and Photometry of asteroids with the Wide Angle Camera of the OSIRIS two-camera system instrument on board the European Space Agency's Rosetta mission. He obtained the PhD title of Doctor in Space Science and Technologies at the University of Padua in 2005. The thesis regarded "A new model of cometary dust and the Wide Angle Camera of the Rosetta Mission". After post-docs in Switzerland, Spain, and Italy, he is now working at the Center of Studies and Activities for Space (CISAS) 'G. Colombo' of the University of Padua. His main research field is the observational study and theoretical modelling of the dust environment in comets.[1]

Asteroid 95008 Ivanobertini

Asteroid 95008 Ivanobertini (2002 AH₁), a background asteroid in the asteroid belt, was named in his honor. The asteroid was discovered at the Italian Cima Ekar Observing Station on 4 January 2002, by the Asiago-DLR Asteroid Survey of which Ivano Bertini has been an active member.[1] The official naming citation was published by the Minor Planet Center on 6 January 2007 (M.P.C. 58597).[2]

Publications

• Pre-hibernation performances of the OSIRIS cameras onboard the Rosetta spacecraft. Magrin et al. Astronomy & Astrophysics, Volume 574, id.A123, 13 pp. (2015)
• Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun. Rotundi et al. Science, Volume 347, Issue 6220, article id. aaa3905. (2015).
• On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko. Sierks et al. Science, Volume 347, Issue 6220, article id. aaa1044. (2015).
• The morphological diversity of comet 67P/Churyumov-Gerasimenko. Thomas et al. Science, Volume 347, Issue 6220, article id. aaa0440. (2015).
• 67P/Churyumov-Gerasimenko: Activity between March and June 2014 as observed from Rosetta/OSIRIS. Tubiana et al. Astronomy & Astrophysics, Volume 573, id.A62, 11 pp. (2014).
• The rotation state of 67P/Churyumov-Gerasimenko from approach observations with the OSIRIS cameras on Rosetta. Mottola et al. Astronomy & Astrophysics, Volume 569, id.L2, 5 pp. (2014).
• Phobos as a D-Type Captured Asteroid, Spectral Modeling from 0.25 to 4.0 μm. Pajola et al. The Astrophysical Journal, Volume 777, Issue 2, article id. 127, 6 pp. (2013).
• Asteroids Close-Up: What We Have Learned from Twenty Years of Space Exploration. Bertini I. In 'Asteroids. Prospective Energy and Material Resources'. Viorel Badescu Editor. Springer (2013).
• Spectrophotometry investigation of Phobos with the Rosetta OSIRIS-NAC camera and implications for its collisional capture. Pajola et al. MNRAS, Volume 427, Issue 4, 3230–3243 (2012).
• Search for satellites near (21) Lutetia using OSIRIS/Rosetta images. Bertini I. et al. Planetary and Space Science, Volume 66, Issue 1, 64-70 (2012).
• Crossing barriers in planetesimal formation: The growth of mm-dust aggregates with large constituent grains. Jankowski T. et al. Astronomy and Astrophysics 542, A80 (2012)
• Photometric observations of comet 81P/Wild 2 during the 2010 perihelion passage. Bertini I. et al. Astronomy and Astrophysics 541, A159 (2012).
• Images of Asteroid 21 Lutetia: A Remnant Planetesimal from the Early Solar System. Sierks H. et al. Science 334, 487-490 (2011).
• Main Belt Comets: A new class of small bodies in the solar system. Bertini I. Planetary and Space Science, Volume 59, Issues 5-6, 365-377 (2011).
• E-Type Asteroid (2867) Šteins as Imaged by OSIRIS on Board Rosetta. Keller H. U. et al. Science 327, 190-193 (2010).
• Coma Structures in Comet 73P/Schwassmann-Wachmann 3, Components B and C, Between January and May 2006. Vincent J-B. et al. Earth, Moon, and Planets, Volume 106, Issue 1, 27-35 (2010).
• The influence of the monomer shape in the first stage of dust growth in the protoplanetary disk. Bertini I. et al. Astronomy and Astrophysics Volume 504, 625-633 (2009).
• Activity evolution, outbursts, and splitting events of comet 73P/Schwassmann-Wachmann 3. Bertini I. et al. Astronomy and Astrophysics, Volume 496, 235-247 (2009).
• Modeling of the light scattering properties of cometary dust using fractal aggregates. Bertini I. et al. Astronomy and Astrophysics, Volume 461, Issue 1, January I 2007, 351-364 (2007).
• Observations of Comet 9P/Tempel 1 around the Deep Impact event by the OSIRIS cameras onboard Rosetta. Keller H. U. et al. Icarus, Volume 187, Issue 1, 87-103 (2007).
• A large dust/ice ratio in the nucleus of comet 9P/Tempel 1. Kuppers M. et al. Nature, Volume 437, Issue 7061, 987-990 (2005).
• A portrait of 4979 Otawara, target of the Rosetta space mission. Fornasier S. et al. Astronomy and Astrophysics, Volume 398, 327-333 (2003).

See also

• Asteroid 21 Lutetia
• Asteroid 2867 Steins
• Asteroid 4979 Otawara
• Comet 73P/Schwassmann–Wachmann (Schwassmann–Wachmann 3)
• Comet 81P/Wild (Wild 2)
• Comet 9P/Tempel 1 (Tempel 1)
• Main-belt comet
• Martian moon Phobos

References

1. "95008 Ivanobertini (2002 AH1)". Minor Planet Center. Retrieved 26 May 2018.
2. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 May 2018.

External links

• JPL Small-Body Database Browser on 95008 Ivanobertini
• The Asiago-DLR Asteroid-Survey
• OSIRIS - The Scientific Imaging System for Rosetta
• ESA Rosetta Mission
• Book 'Asteroids. Prospective Energy and Material Resources'. Viorel Badescu Editor. Springer (2013)