Feeling the Pressure: Effects of Formation Pressure on the Physical Properties of Titan Haze Analogs
The Cassini–Huygens mission detected large negative ions in Titan’s ionosphere at pressures as low as 10 ^−6 Torr. These ions ultimately polymerize to form Titan’s complex organic haze particles, which are observed throughout the atmosphere and potentially on the surface. Laboratory analogs of thes...
I tiakina i:
| Ngā kaituhi matua: | , , , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2026-01-01
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| Rangatū: | The Planetary Science Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/PSJ/ae63ca |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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