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Relación estadística orto-para del agua desorbida del hielo a 10 kelvin
Tetsuya Hama1, Akira Kouchi2, Naoki Watanabe2
1Institute of Low Temperature Science, Hokkaido University, Sapporo 060-0819, Japan. hama@lowtem.hokudai.ac.jp.
Resumen
Agua gaseosa
Área de la Ciencia:
- Astroquímica
- Física del medio interestelar
- Ciencias planetarias
Sus antecedentes:
- La relación orto-para (OPR) del agua se utiliza para inferir las temperaturas de formación de hielo en el espacio.
- Este método asume que el OPR del agua refleja su temperatura de formación de hielo en los granos de polvo.
Objetivo del estudio:
- Investigar la relación entre la relación orto-para (OPR) del agua y su temperatura de formación de hielo.
- Reevaluar el uso de OPR para determinar las temperaturas de formación de hielo interestelar.
Principales métodos:
- Formación de hielo in situ por hidrogenación de O2 a 10 grados Kelvin.
- Medición del OPR de las moléculas de agua desorbida.
Principales resultados:
- El agua desorbida del hielo de 10 Kelvin exhibió un alto OPR de 3, inconsistente con las bajas temperaturas de formación.
- Este hallazgo desafía la suposición de que el OPR del agua se correlaciona directamente con la temperatura de formación de hielo.
Conclusiones:
- La relación asumida entre el OPR del agua y la temperatura de formación de hielo es inválida.
- La reinterpretación de los OPR bajos es crucial para comprender la historia química del agua interestelar y los primeros procesos del sistema solar, incluida la formación de cometas.
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