By observing infrared light, which is less affected by cosmic
dust than visible light, and exploiting the excellent conditions at ESO's Paranal Observatory, the team was able to get a clearer view of this region than ever before.
Not exact matches
Infrared radiation passes through interstellar
dust much more easily
than visible light, so by looking at the infrared
light from a galaxy we can learn about the new stars forming within the clouds of
dust and gas.
In fact it's positively chilly, with more
than half the energy emitted by normal matter coming from clouds of gas and
dust too cold to radiate
visible light — and which therefore can not be seen with traditional telescopes.
For the same reason, infrared astronomy enables researchers to observe cosmic objects through large clouds of interstellar
dust that scatter infrared radiation substantially less
than visible light.
While probing space in depth — let us bear in mind that the further we look, the more we go back in time — ALMA detects the glow of tepid
dust present in the most distant galaxies, i.e., the earliest ones, with better resolution
than could be possible in the deepest observations using
visible or infrared
light.