Spectroscopic anatomy of a meteor trail cross section with the European Southern Observatory Very Large Telescope

Details Spectroscopic anatomy of a meteor trail cross section with the European Southern Observatory Very Large Telescope Spectroscopic anatomy of a meteor trail cross section with the European Southern Observatory Very Large Telescope

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004m%26ps...39..609j&link_type=abstract

Meteoritics & Planetary Science, Vol. 39, No. 4, p.609-616

Physics

4

Scientific paper

A meteor spectrum was recorded serendipitously at the European Southern Observatory (ESO) Very Large Telescope (VLT) during a long exposure in long-slit spectroscopic mode with FORS1. The -8 magnitude fireball crossed the narrow 1 × 7 slit during the observation of a high z supernova in normal service mode operation on May 12, 2002. The spectrum covered the range of 637-1050 nm, where the meteor's air plasma emissions from N2, N, and O dominate. Carbon atom emission was not detected in the relatively unexplored wavelength range above 900 nm, but the observed upper limit was only 3 sigma less than expected from the dissociation of atmospheric CO2. The meteor trail was resolved along the slit, and the emission had a Gaussian distribution with a dimension of FWHM = 7.0 (±0.4) * sin(a) * H (km)/90 m, where a is the unknown angle between the orientation of the meteor path and slit and H the assumed altitude of the meteor in km. To our knowledge, this is the first observation of a spatially resolved spectrum across a meteor trail. Unlike model predictions, the plasma excitation temperature varied only from about 4,300 to 4,365 K across the trail, based on the ratio of atomic and molecular nitrogen emissions. Unfortunately, we conclude that this was because the meteor at 100 km altitude was out of focus.

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