Washington: Astronomers have taken the first-ever image of a snow line in an infant solar system.
This frosty landmark is believed to play an essential role in the formation and chemical make-up of planets around a young star.
On Earth, snow lines typically form at high elevations where falling temperatures turn atmospheric moisture to snow similarly snow lines are believed to form around young stars in the distant, colder reaches of the disks from which solar systems form.
Depending on the distance from the star, however, other more exotic molecules can freeze and turn to snow.
Familiar water ice freezes out first, then moving outward in concentric circles other abundant gases like carbon dioxide (CO2), methane (CH4), and carbon monoxide (CO) freeze, forming a frost on dust grains, which are the building blocks of planets and comets.
Atacama Large Millimeter/submillimeter Array (ALMA) telescope spotted a never-before-seen CO snow line around TW Hydrae, a young star 175 light-years away from Earth.
Astronomers believe this nascent solar system has many of the same characteristics that our own solar system had when it was just a few million years old.
Chunhua "Charlie" Qi, a researcher with the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts, said the team can now see previously hidden details about the frozen outer reaches of another solar system, one that has much in common with our own when it was less than 10 million years old.
Snow lines have, until now, only been detected by their spectral signatures; they have never been imaged directly, so their precise location and extent could not be determined.
This is because snow lines form exclusively in the relatively narrow central plane of a protoplanetary disk. Above and below this region, stellar radiation keeps the gases warm, preventing them from forming ice.
Only with the insulating effect of the concentrated dust and gas in the central plane of the disk can temperatures drop sufficiently for CO and other gases to cool and freeze.
Normally, this outer cocoon of hot gas would prevent astronomers from peering inside the disk where the gas had frozen out. "It would be like trying to find a small, sunny patch hidden within a dense fogbank," said Karin Oberg, a researcher with Harvard University and the University of Virginia in Charlottesville.
The astronomers were able to pierce the intervening CO fog by instead hunting for a different molecule known as diazenylium (N2H+). This fragile molecule is easily destroyed in the presence of CO gas, so would only appear in detectable amounts in regions where CO had frozen out, and is hence a proxy for CO ice.
Diazenylium shines brightly in the millimeter portion of the spectrum, which can be detected by radio telescope like ALMA here on Earth.
Snow lines, astronomers believe, serve a vital role in the formation of a solar system. They help dust grains overcome their normal tendency to collide and self-destruct by giving the grains a stickier outer coating.
They also increase the amount of solids available and may dramatically speed up the planet formation process. Since there are multiple snow lines, each may be linked to the formation of specific kinds of planets.
Around a Sun-like star, the water snow line would correspond approximately to the orbit of Jupiter and the CO snow line would roughly correspond to the orbit of Neptune. The transition to CO ice could also mark the starting point where smaller icy bodies like comets and dwarf planets like Pluto would form.
Oberg also points out that the CO snow line is particularly interesting since CO ice is needed to form methanol, which is a building block of more complex organic molecules that are essential for life. Comets and asteroids could then ferry these molecules to newly forming Earth-like planets, seeding them with the ingredients for life.
The results have been published in Science Express.
ANI
