3.3 micron emission from ultraviolet excitation of some aromatic molecules

3.4 Micron Emission from Aliphatic Hydrocarbons in Proto-Planetary Nebulae

3.45 b.y.-old microbial associations in cherts from the Pilbara: lessons for potential Martian life

3.6 years of DIRBE NIR stellar light curves (Price+, 2010)

30 DENIS late-M dwarfs between 15 and 30pc (Phan-Bao+, 2001)

30,000 Years of Hydrothermal Activity at the Lost City Vent Field

30th Lunar and Planetary Science Conference: Some Highlights

31 Cygni: The B star and the wind

318-MHz variability of complete samples of extragalactic radio sources

32 GHz point source observations for decontaminating CBI2 CMB and SZE cluster fields

320x240 pixel InGaAs/InP focal plane array for short-wave infrared and visible light imaging

325MHz radio survey in M31. II. (Gelfand+, 2005)

32GHz point source observations for decontaminating CBI2 CMB and SZE cluster fields - 2

32Si in precipitation: evaluation of temporal and spatial variation and as dating tool for glacial ice

330-360GHz spectral lines of G 34.3+0.15. (Macdonald+, 1996)

34S/32S ratios for the different forms of sulphur in the Orgueil meteorite and their mode of formation

3820 Ma zircons from a tonalitic Armîsoq gneiss in the Godthåb district of Southern West Greenland

39 Ar- 40 Ar dating of two lunar granites: The age of Copernicus

39Ar - 40Ar age of the Ibitira eucrite and constraints on the time of pyroxene equilibration.

39Ar -40Ar Ages of Two Nakhlites, MIL 03346 and Y 000593: A Detailed Analysis