Editing Hydroxy group (section)

===Atmosphere of Venus===
The [[Venus Express]] orbiter collected [[Venus]] science data from April 2006 until December 2014. In 2008, Piccioni, ''et al.'' reported measurements of night-side airglow emission in the atmosphere of Venus made with the Visible and Infrared Thermal Imaging Spectrometer (VIRTIS) on Venus Express. They attributed emission bands in wavelength ranges of 1.40–1.49&nbsp;micrometers and 2.6–3.14 micrometers to vibrational transitions of OH.<ref name="Piccioni Drossart Zasova Migliorini 2008 pp. L29–L33">{{cite journal |last1=Piccioni |first1=G. |last2=Drossart |first2=P. |last3=Zasova |first3=L. |last4=Migliorini |first4=A. |last5=Gérard |first5=J.-C. |last6=Mills |first6=F. P. |last7=Shakun |first7=A. |last8=García Muñoz |first8=A. |last9=Ignatiev |first9=N. |last10=Grassi |first10=D. |last11=Cottini |first11=V. |last12=Taylor |first12=F. W. |last13=Erard |first13=S. |title=First detection of hydroxyl in the atmosphere of Venus |journal=Astronomy & Astrophysics |publisher=EDP Sciences |volume=483 |issue=3 |date=2008-04-01 |issn=0004-6361 |doi=10.1051/0004-6361:200809761 |pages=L29–L33|doi-access=free |bibcode=2008A&A...483L..29P |hdl=1885/35639 |hdl-access=free }}</ref> This was the first evidence for OH in the atmosphere of any planet other than Earth.<ref name="Piccioni Drossart Zasova Migliorini 2008 pp. L29–L33"/>