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http://cio.repositorioinstitucional.mx/jspui/handle/1002/703| Extrasolar planet observatory on the far side of the moon | |
| MARIJA STROJNIK POGACAR | |
| En Embargo | |
| 30-06-2019 | |
| Atribución-NoComercial-SinDerivadas | |
| We define the simplest signal-to-noise ratio (SNR) to determine the optimal wavelength interval for extrasolar planet detection. We expand the width of the spectral region from infrared up to submillimeter range. For a nearby solar system similar to our own, we find that the SNR increases by about 100 in comparison to that considered previously. We propose the planet detection in a spectral interval around 0.3 mm (900 GHz), in which we evaluate the SNR to be 10–4. We perform trade-off analysis for alternative sites for the planet observatory, concluding that the far side of the moon offers a most favorable, atmosphere-free environment and a stable base. | |
| 2014-06 | |
| Artículo | |
| CIENCIAS FÍSICO MATEMÁTICAS Y CIENCIAS DE LA TIERRA | |
| Aparece en las colecciones: | Articulos Arbitrados 2014 |