EDP Sciences
Free Access
Issue
A&A
Volume 425, Number 3, October III 2004
Page(s) 1119 - 1124
Section Planets and planetary systems
DOI https://doi.org/10.1051/0004-6361:20040477


A&A 425, 1119-1124 (2004)
DOI: 10.1051/0004-6361:20040477

Detection of neutral sodium above Mercury during the transit on 2003 May 7

H. Schleicher1, G. Wiedemann2, H. Wöhl1, T. Berkefeld1 and D. Soltau1

1  Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany
    e-mail: schleicher@kis.uni-freiburg.de
2  Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany

(Received 19 March 2004 / Accepted 1 June 2004)

Abstract
The extent of the exosphere of Mercury above the planet's limb could for the first time be observed by detecting an excess absorption in the solar sodium line D 2 during the transit of Mercury across the solar disk on 2003 May 7. The observations were performed with a 2d Fabry-Perot spectrograph of the Vacuum Tower Telescope at Izaña, Tenerife. The absorption excess, blue-shifted by 13 pm relative to the solar line, is mainly concentrated near the polar regions. There, the absorption excess can be traced up to $\approx$ 700 km above the limb. Between the two polar regions, along the eastern limb, a weaker absorption excess can be seen. A possible streamer-like feature stretches more than 2000 km above the northern region. Assuming the density to decrease exponentially with height, we derive for the polar maxima vertical column densities of 3  $\times$ $10^{10}~{\rm cm}^{-2}$, volume densities at the surface of 2.5  $\times$ $10^3~{\rm cm}^{-3}$, and a density scale height of 150 km.


Key words: planets and satellites: individual: Mercury




© ESO 2004