Phosphine signature in Venus’s spectrum

This artistic representation shows a real image of Venus, taken with ALMA, in which ESO is a partner, with two superimposed spectra taken with ALMA (in white) and the James Clerk Maxwell Telescope (JCMT; in grey). 

The dip in Venus’s JCMT spectrum provided the first hint of the presence of phosphine on the planet, while the more detailed spectrum from ALMA confirmed that this possible marker of life really is present in the Venusian atmosphere.

As molecules of phosphine float in the high clouds of Venus, they absorb some of the millimetre waves that are produced at lower altitudes. When observing the planet in the millimetre wavelength range, astronomers can pick up this phosphine absorption signature in their data, as a dip in the light from the planet.

Telif:

ALMA (ESO/NAOJ/NRAO), Greaves et al. & JCMT (East Asian Observatory)

Görüntü Hakkında

Kimlik:eso2015f
Tür:Gezegene ait
Yayın tarihi:14 Eylül 2020 17:00
Bağlantılı bültenler:eso2015
Boyut:890 x 890 px

Nesne Hakkında

Adı:Venus
Tür:Solar System : Planet : Feature : Atmosphere
Kategori:Solar System

Görüntü Türleri

Büyük JPEG
73,6 KB

Yaklaştırma


Duvarkağıtları

1024x768
82,2 KB
1280x1024
108,5 KB
1600x1200
141,4 KB
1920x1200
164,9 KB
2048x1536
194,8 KB