Mouser Megan D
Jacobs Technology, NASA Johnson Space Center, Houston, TX, USA.
Nat Commun. 2024 Jun 14;15(1):5062. doi: 10.1038/s41467-024-49497-2.
Surface observations suggest that carbon may exist in Mercury’s interior. Under planetary mantle pressures and temperatures, carbon may be present as a stable diamond layer which may have important implications for the physical and chemical properties of Mercury.
地面观测表明碳可能存在于水星内部。在行星地幔的压力和温度条件下,碳可能以稳定的钻石层形式存在,这可能对水星的物理和化学性质具有重要意义。