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Laboratory of Astrophysics & Surface Science

The laboratory is located in the Physics Building of Syracuse University; it is headed by Prof. Vidali. His group consists of graduate and undergraduate students, a post-doc and external collaborators. For a list of current collaborators, see the "Team" entry on the left menu.

The current main research project is the study of physical and chemical processes in the interstellar medium and in planetary atmospheres. The group uses tools that were employed in the research of properties of solid surfaces (atom-surface interaction, surface morphology, phase transitions in ultra-thin films, thin film growth). These tools include: ultra=high vacuum techniques, atomic/molecular beams, low temperature techniques, mass s[ectrometry, in-situ infrared spectroscopy (RAIRS); laser spectroscopy (REMPI), LEED/Auger, Atom Force Microscopy (AFM), and MBE/vapor deposition of solid films.

There are four main directions in his group's research:

  • The study of processes leading to the formation of molecular hydrogen on interstellar dust grain analogues in conditions relevant to astrophysical environments;
  • The study of oxidation/hydrogenation reactions in/on interstellar ices and bare dust grain analogs;
  • The study of formation of precursors to biogenic material on interstellar ice analogues;
  • The study of the formation of biogenic molecules in planetary atmospheres, such as the atmosphere of Titan, the satellite of Saturn.

Prof. Vidali's research has been written up in Scientific American Online, The Washington Post - online, Popular Mechanics, Nature News - online, Chemical Engineering News, Il Sole 24 Ore, and others.
The latest publications:
  • D.Jing, J.He, J.Brucato, A.De Sio, L.Tozzetti, and G.Vidali: "On water formation in the interstellar medium: laboratory study of the O+D reaction on surfaces", Astrophys. J. Lett. 741, L9 (2011).
  • J.He, P.Frank, and G.Vidali: "Interaction of hydrogen with surfaces of silicates: single crystal vs. amorphous", Phys.Chem.Chem.Phys. 13, 15803 (2011).
  • J.L Lemaire, G.Vidali, S. Baouche, M.Chehrouri, H.Chaabouni, and H.Mokrane: "Competing mechanisms of molecular hydrogen formation in conditions relevant to the interstellar medium", Astrophys. J. Lett. , 725, 126 (2010)
  • L.Li, H.Zhao, G.Vidali, Y.Frank, I.Lohmar, H.B.Perets, and O.Biham: "Interac- tion of Atomic and Molecular Hydrogen with Tholin Surfaces at Low Temperatures", J.Phys.Chem. A 114, 10575 (2010).
  • J.He, K.Gao, G.Vidali, C.J.Bennett, and R.I.Kaiser: "Formation of molecular hydrogen desorption from methane ice", Astropys. J. 721, 1656 (2010)
  • G.Vidali and L.Li: "Molecular hydrogen desorption from amorphous surfaces at low temperature", J. Phys.: Condens. Matter 22 (2010) 304012.
  • S,Madzunkov, J.MacAskill, A .Chutjian, P.Ehrenfreund, M.Darrach, G.Vidali, and B.J.Shortt: "Formation of H2CO and CO2 on an icy grain analogue using fast H atoms", J. Phys.: Conference Series 194, 092005 (2009)
  • G.Vidali, G., L. Li, J.E., Roser, and R. Badman: Catalytic Activity of Interstellar Grains: Formation of Molecular Hydrogen on Amorphous Silicates Adv.Space Res. 43, 1291(2009).

For a complete list, see the link at left.

For an introduction to his research, here are the slides from recent presentations given by Prof. Vidali:

Other presentations:
  • Interstellar Medium Physics and Chemistry Colloquium at Syracuse University, Physics Department (November 2002) (pdf file)
  • In this invited presentation (in PowerPoint format) at the American Chemical Society National Meeting in Boston, Mass. (August 2002) Description of research on hydrogen recombination reactions on several interstellar dust grain analogues and on the oxidation of carbon monoxide ice by oxygen atoms.
  • Lay-language paper about hydrogen recombination on interstellar dust grains. It was prepared for a press conference held on March 24, 1999 at the American Physical Society Centennial Meeting in Atlanta (html)



  • Questions? Contact Prof. Vidali

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