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A&A 429, L41-L45 (2005)
DOI: 10.1051/0004-6361:200400102
Letter
Gamma-ray bursts and other sources of giant lightning discharges in protoplanetary systems
B. McBreen1, E. Winston1, S. McBreen2 and L. Hanlon11 Department of Experimental Physics, University College, Dublin 4, Ireland
e-mail: brian.mcbreen@ucd.ie
2 Astrophysics Missions Division, Research Scientific Support Department of ESA, ESTEC, Noordwijk, The Netherlands
(Received 23 June 2004 / Accepted 6 November 2004)
Abstract
Lightning in the solar nebula is considered to be one
of the probable sources for producing the chondrules that are
found in meteorites. Gamma-ray bursts (GRBs) provide a large
flux of
-rays that Compton scatter and create a charge
separation in the gas because the electrons are displaced from
the positive ions. The electric field easily exceeds the
breakdown value of
1 V m
-1 over distances of order
0.1 AU. The energy in a giant lightning discharge exceeds a
terrestrial lightning flash by a factor of ~10
12. The
predicted post-burst emission of
-rays from accretion
into the newly formed black hole or spin-down of the magnetar is
sufficiently intense to cause a lightning storm in the nebula
that lasts for days and is more probable than the GRB because the
radiation is beamed into a larger solid angle. The giant
outbursts from nearby soft gamma-ray repeater sources (SGRs) are
also capable of causing giant lightning discharges. The total
amount of chondrules produced is in reasonable agreement with the
observations of meteorites. Furthermore in the case of GRBs most
chondrules were produced in a few major melting events by nearby
GRBs and lightning occurred at effectively the same time over the
whole nebula, and provide accurate time markers to the formation
of chondrules and evolution of the solar nebula. This model
provides a reasonable explanation for the delay between the
formation of calcium aluminium inclusions (CAIs) and chondrules.
Key words: gamma rays: bursts -- solar system: formation -- planetary systems: protoplanetary disks -- planetary systems: formation
SIMBAD Objects
© ESO 2005
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