説明
Traces of 2-3 Myr old 60Fe were recently discovered in a manganese crust and in lunar samples. We have found that this signal is extended in time and is present in globally distributed deep-sea archives. A second 6.5-8.7 Myr old signature was revealed in a manganese crust. The existence of the Local Bubble hints to a recent nearby supernova-activity starting 13 Myr ago. With analytical and numerical models generating the Local Bubble, we explain the younger 60Fe-signature and thus link the evolution of the solar neighborhood to terrestrial anomalies.
4 pages, 3 figures, accepted for publication in JPS Conf. Proc
収録刊行物
-
- Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016)
-
Proceedings of the 14th International Symposium on Nuclei in the Cosmos (NIC2016) 2017-02-27
Journal of the Physical Society of Japan
- Tweet
キーワード
- deep-sea samples
- interstellar medium
- Earth and Planetary Astrophysics (astro-ph.EP)
- astro-ph.SR
- 103014 Kernphysik
- Fe-60
- FOS: Physical sciences
- SUPERNOVAE
- 103004 Astrophysik
- Al-26
- Astrophysics - Solar and Stellar Astrophysics
- astro-ph.EP
- supernova
- accelerator mass spectrometry
- Local Bubble
- 103004 Astrophysics
- 103014 Nuclear physics
- Solar and Stellar Astrophysics (astro-ph.SR)
- Astrophysics - Earth and Planetary Astrophysics
詳細情報 詳細情報について
-
- CRID
- 1871146592795677824
-
- データソース種別
-
- OpenAIRE