A new ultrahigh vacuum experiment is described to study atom and radical addition reactions in interstellar ice analogues for astronomically relevant temperatures. The new setup – SURFace REaction SImulation DEvice (SURFRESIDE2) – allows a systematic investigation of solid state pathways resulting in the formation of molecules of astrophysical interest. The implementation of a double beam line makes it possible to expose deposited ice molecules to different atoms and/or radicals sequentially or at the same time. Special efforts are made to perform experiments under fully controlled laboratory conditions, including precise atom flux determinations, in order to characterize reaction channels quantitatively. In this way, we can compare and combine different surface reaction channels with the aim to unravel the solid state processes at play in space. Results are constrained in situ by means of a Fourier transform infrared spectrometer and a quadrupole mass spectrometer using reflection absorption infrared spectroscopy and temperature programmed desorption, respectively. The performance of the new setup is demonstrated on the example of carbon dioxide formation by comparing the efficiency through two different solid state channels (CO + OH → CO2 + H and CO + O → CO2) for which different addition products are needed. The potential of SURFRESIDE2 to study complex molecule formation, including nitrogen containing (prebiotic) compounds, is discussed.
Skip Nav Destination
Article navigation
July 2013
Research Article|
July 24 2013
SURFRESIDE2: An ultrahigh vacuum system for the investigation of surface reaction routes of interstellar interest
S. Ioppolo;
S. Ioppolo
a)
1Sackler Laboratory for Astrophysics, Leiden Observatory,
Leiden University
, P.O. Box 9513, 2300 RA Leiden, The Netherlands
Search for other works by this author on:
G. Fedoseev;
G. Fedoseev
1Sackler Laboratory for Astrophysics, Leiden Observatory,
Leiden University
, P.O. Box 9513, 2300 RA Leiden, The Netherlands
Search for other works by this author on:
T. Lamberts;
T. Lamberts
1Sackler Laboratory for Astrophysics, Leiden Observatory,
Leiden University
, P.O. Box 9513, 2300 RA Leiden, The Netherlands
2Institute for Molecules and Materials,
Radboud University Nijmegen
, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
Search for other works by this author on:
C. Romanzin;
C. Romanzin
3Laboratoire de Chimie Physique,
UMR 8000 CNRS-Université Paris Sud
, 91405 Orsay, France
Search for other works by this author on:
H. Linnartz
H. Linnartz
b)
1Sackler Laboratory for Astrophysics, Leiden Observatory,
Leiden University
, P.O. Box 9513, 2300 RA Leiden, The Netherlands
Search for other works by this author on:
a)
Current address: Division of Geological and Planetary Sciences, California Institute of Technology, 1200 E. California Blvd., Pasadena, California 91125, USA. Electronic mail: [email protected]
b)
Electronic mail: [email protected]
Rev. Sci. Instrum. 84, 073112 (2013)
Article history
Received:
March 04 2013
Accepted:
July 08 2013
Citation
S. Ioppolo, G. Fedoseev, T. Lamberts, C. Romanzin, H. Linnartz; SURFRESIDE2: An ultrahigh vacuum system for the investigation of surface reaction routes of interstellar interest. Rev. Sci. Instrum. 1 July 2013; 84 (7): 073112. https://doi.org/10.1063/1.4816135
Download citation file:
Pay-Per-View Access
$40.00
Sign In
You could not be signed in. Please check your credentials and make sure you have an active account and try again.
Citing articles via
An instrumentation guide to measuring thermal conductivity using frequency domain thermoreflectance (FDTR)
Dylan J. Kirsch, Joshua Martin, et al.
Overview of the early campaign diagnostics for the SPARC tokamak (invited)
M. L. Reinke, I. Abramovic, et al.
Analysis methodology of coherent oscillations in time- and angle-resolved photoemission spectroscopy
Nicolas Gauthier, Hadas Soifer, et al.
Related Content
A cryogenic ice setup to simulate carbon atom reactions in interstellar ices
Rev. Sci. Instrum. (May 2020)
Water formation by surface O3 hydrogenation
J. Chem. Phys. (February 2011)
Oxygen diffusion and reactivity at low temperature on bare amorphous olivine-type silicate
J. Chem. Phys. (February 2014)
Water formation through O2 + D pathway on cold silicate and amorphous water ice surfaces of interstellar interest
J. Chem. Phys. (December 2012)