Spectroscopic anatomy of a meteor trail cross section with the European Southern Observatory Very Large Telescope
dc.contributor.author | Jenniskens, P | |
dc.contributor.author | Jehin, E | |
dc.contributor.author | Cabanac, RA | |
dc.contributor.author | Laux, CO | |
dc.contributor.author | Boyd, ID | |
dc.date.accessioned | 2025-01-21T01:08:11Z | |
dc.date.available | 2025-01-21T01:08:11Z | |
dc.date.issued | 2004 | |
dc.description.abstract | 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" x 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 N-2, N, and 0 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(alpha) * H (km)/90 m, where alpha 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. | |
dc.fuente.origen | WOS | |
dc.identifier.eissn | 1945-5100 | |
dc.identifier.issn | 1086-9379 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/96437 | |
dc.identifier.wosid | WOS:000221017100008 | |
dc.issue.numero | 4 | |
dc.language.iso | en | |
dc.pagina.final | 616 | |
dc.pagina.inicio | 609 | |
dc.revista | Meteoritics & planetary science | |
dc.rights | acceso restringido | |
dc.title | Spectroscopic anatomy of a meteor trail cross section with the European Southern Observatory Very Large Telescope | |
dc.type | artículo | |
dc.volumen | 39 | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |