Abstract
We present a model for the outburst of supernova SN1987A. This supernova was discovered in the Large Magellanic Cloud on 24 February, 1987. Astrometry1,2 reveals the supernova to lie within 0.1 arcs of the B3 I supergiant Sanduleak (Sk) –69 202. The optical features indicate that the event was a type II supernova. Such supernovae are the expected consequence of the evolution of massive stars M >=10M⊙ and may be expected to leave behind a neutron star or black-hole remnant. Neutrinos released as a consequence of the anticipated core collapse to neutron star densities may indeed have been observed (ref. 3; Aglietta et al. preprint, 1987; Bionta et al. preprint, 1987). SN1987A certainly cannot be considered a prototype of a type II supernova, however, as it has proved to be unusual in several respects, including: (1) the progenitor of SN1987A appears to have been a blue supergiant rather than a red supergiant star; (2) SN1987A was found to be some 3 or 5 magnitudes dimmer at visual maximum than is known to be typical of supernovae of type II; and (3) SN1987A exhibited an extremely rapid spectral development, seemingly consistent with the very high expansion velocities inferred from studies of the hydrogen absorption features in the early spectra. Here we present a model for the outburst of SN1987A that permits a straightforward interpretation of the observed behaviour.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
1. West, R. M., Laubetts, A., J0rgensen, H. E. & Schuster, H. E. Astr. Astrophys. (submitted). 2. White, G. L. & Malin, D. F. IAU Ore. No. 4330 (1987); Nature 327, 36–38 (1987). 3. Hirata, et al. Phys Rev. Lett, (submitted). 4. Sonneborn, G. & Kirshner, R. IAU Circ. No. 433 (1987). 5. Panagia, W. et al. Astr. Astrophys. (in the press). 6. Brunish, W. E. & Truran, J. W. Astrophys. J. Suppl. Ser. 49, 447–468 (1982). 7. Kippenhahn, R., Weigert, A. & Hofmeister, E. in Methods in Computational Physics, Vol. 7 (eds Alder, B., Fernbach, S. & Rotenberg, M.) 129–190 (Academic, New York, 1967). 8. Weiss, A. Astr. Astrophys. (in the press). 9. Hiibner, W. F., Merts, H. L., Magee, N. H. Jr & Argo, M. F. Los Alamos Sci. Lab. Rep. LA 6760 M (1977). 10. Chiosi, C. & Maeder, A. A Rev. Astr. Astrophys. 24, 329–375 (1987). 11. Falk, S. W. & Arnett, W. D. Astrophys. J. Suppl. Ser. 33, 515–562 (1977). 12. Sedov, L. I. Similarity and Dimensional Methods in Mechanics 260 (Academic, New York, 1959). 13. Wilson, J. R., Mayle, R., Woosley, S. E. & Weaver, T. Ann. N. Y. Acad. Sci. (in the press). 14. Woosley, S. A. & Weaver, T. A. A. Rev. Astr. Astrophys. 24, 205–293 (1986). 15. Thielemann, F. K. & Arnett, W. D. Astrophys. J. 295, 604–619 (1985).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Hillebrandt, W., Höflich, P., Truran, J. et al. Explosion of a blue supergiant: a model for supernova SN1987A. Nature 327, 597–600 (1987). https://doi.org/10.1038/327597a0
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/327597a0
This article is cited by
-
The dusty and extremely red progenitor of the type II supernova 2023ixf in Messier 101
Science China Physics, Mechanics & Astronomy (2024)
-
SN 1987A and SN 1993J: Testing stellar evolution theory?
Space Science Reviews (1994)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.