C.D.S. - SIMBAD4 rel 1.7 - 2020.07.03CEST22:03:03

2018A&A...616A..85P - Astronomy and Astrophysics, volume 616A, 85-85 (2018/8-1)

The consequences of a nearby supernova on the early solar system.


Abstract (from CDS):

If the Sun was born in a relatively compact open cluster (half-mass radius ≤3pc) with ≥103 stars, it is quite likely that a massive (≥10M) star was nearby when it exploded in a supernova. The repercussions of a supernova can be rather profound, and the current solar system may still bear the scars of this traumatic event. The truncation of the Kuiper belt and the tilt of the ecliptic plane with respect to the Sun's rotation axis could represent such signatures. We simulated the effect of a nearby supernova on the young solar system using the Astrophysical Multipurpose Software Environment (AMUSE). Our calculations are realized in two subsequent steps in which we study the effect of the supernova irradiation on the circumstellar disk and the effect of the impact of the nuclear blast-wave which arrives a few decades later. We find that the blast wave of our adopted supernova exploding at a distance of 0.15-0.40pc and at an angle of 35°-65° with respect to the angular-momentum axis of the circumsolar disk would induce a misalignment between the Sun's equator and its disk to 5.6°±1.2°, consistent with the current value. The blast of a supernova truncates the disk at a radius between 42 and 55au, which is consistent with the current edge of the Kuiper belt. For the most favored parameters, the irradiation by the supernova as well as the blast wave heat the majority of the disk to ≥1200K, which is sufficiently hot to melt chondrules in the circumstellar disk. The majority of the planetary system may have been affected by a nearby supernova. Some of its repercussions, such as truncation and tilting of the disk, may still be visible in the current planetary system topology. The amount of material from the supernova blast wave that is accreted by the circumstellar disk is too small by several orders of magnitude to explain the current abundance of the short-lived radionuclide 26Al.

Abstract Copyright: © ESO 2018

Journal keyword(s): methods: numerical - planets and satellites: dynamical evolution and stability

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
1 W 3 MoC 02 27 04.10 +61 52 27.1           ~ 962 3
2 PS1-1000001 SN* 03 29 48.735 -29 04 29.91           SNII 2 0
3 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14826 1
4 V* TW Hya TT* 11 01 51.9054298616 -34 42 17.031550898   11.94 10.50 10.626 9.18 K6Ve 1532 1
5 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3027 0
6 PS1-11aof SN* 23 25 59.575 -00 30 55.16           SNIIP 3 0

    Equat.    Gal    SGal    Ecl

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