Ultraviolet spectra of Comet 96/P Machholz were obtained during its 2002 perihelion with the UVCS instrument aboard the SOHO satellite. Emission from H I, C II, C III, and O I, is detected near the nucleus. The outgassing rate is in line with the value extrapolated from rates at larger distances from the Sun, and abundances of C and O are estimated. Reconstructed images show a nearly spherical cloud in H I Lyα emission and an ion tail seen in C III. Radiation pressure on the hydrogen atoms produces a modest distortion of the shape of the Lyα cloud as seen from SOHO, and it produces Doppler shifts up to 30 km s−1 in the outer parts of the cloud. We estimate a ratio of C to H2O similar to what is observed in other comets, so low carbon abundance does not account for the anomalously low C2 and C3 ratios to NH2 observed at optical wavelengths.
@article{arxiv.2111.15644,
title = {Ultraviolet Observations of Comet 96/P Machholz at Perihelion},
author = {J. C. Raymond and S. Giordano and S. Mancuso and M. S. Povich and A. Bemporad},
journal= {arXiv preprint arXiv:2111.15644},
year = {2022}
}