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Brown Dwarf research laying groundwork for exoplanet exploration

Stanimir Metchev shows how Brown Dwarf research enriches exoplanet studies and the search for life
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A comparison of the HR 8799 system and our solar system, showing how dramatically different they are. Note the terrestrial planets are so close to the sun they donSA国际影视传媒檛 even fit on the chart by scale. screenshot courtesy of Aurora Research Institute
A comparison of exoplanets found by the Kepler space telescope showing their relative mass and distance from their respective stars and comparing to Earth. They are named based on the planet that found them, so Kepler-22b and Kepler-186f are in entirely different parts of the galaxy. The number denotes the star and the letter denotes the planet in the solar system. screenshot courtesy of Aurora Research Institute
A comparison of exoplanets found by the Kepler space telescope showing their relative mass and distance from their respective stars and comparing to Earth. They are named based on the planet that found them, so Kepler-22b and Kepler-186f are in entirely different parts of the galaxy. The number denotes the star and the letter denotes the planet in the solar system. screenshot courtesy of Aurora Research Institute

Scientists cannot measure key data on exoplanets yet, so instead theySA国际影视传媒檙e honing their techniques on brown dwarfs.

Astronomer Stanimir Metchev explained ways scientists estimate weather billions of kilometres away and map out exoplanets in a May 4 presentation as part of the Aurora Speaker Series.

Normally the series showcases scientific research completed in the Beaufort Delta to the world, but this time the cosmos came to Inuvik. Each year, the Canadian Astronomy SocietySA国际影视传媒檚 CASCA-Westar Lectureship program allows communities to book an astronomer to come lecture. The idea is to bring more current astronomy knowledge to the general public.

Inuvik had been approved under the program, but had to delay the visit because of the COVID-19 pandemic. So the Aurora Research Institute opted to host the series virtually.

One of the hottest topics in modern astronomy are exoplanets and areas beyond the solar system, which Metchev discussed in detail.

What scientists actually see SA国际影视传媒 because stars emit light and planets donSA国际影视传媒檛, astronomers measure drops in brightness as planets cross the path between the star and Earth and can deduce facts about the planet. This particular image from 2008 is of the star HR 8799 and is the first time exoplanets were found using this method. screenshot courtesy of Aurora Research Institute
What scientists actually see SA国际影视传媒 because stars emit light and planets donSA国际影视传媒檛, astronomers measure drops in brightness as planets cross the path between the star and Earth and can deduce facts about the planet. This particular image from 2008 is of the star HR 8799 and is the first time exoplanets were found using this method. screenshot courtesy of Aurora Research Institute

SA国际影视传媒淭he kinds of stuff that we do in my team at Western University is actually study the atmospheres and believe it or not even the weather patterns on other planets,SA国际影视传媒 said Metchev.

Scientists have identified over 4,700 exoplanets in the last two decades, and about 60 are potential candidates for life. Metchev explained astronomers are currently looking for planets in the habitable or SA国际影视传媒淕oldilocksSA国际影视传媒 zone, an area close enough to the sun where liquid water could exist on the planetSA国际影视传媒檚 surface.

Around a star like our sun, that zone is a bit over 148 million kilometres out. The majority of stars found to have exoplanets so far, however, are red dwarfs. These stars are considerably smaller, cooler and dimmer than our star, so any liquid water would be located a lot closer to the star than in our own solar system. Stars increase with intensity as they move up the colour spectrum, ranging from red to blue.

In spite of this very specific criteria, scientists have a few candidates for SA国际影视传媒淓arthlikeSA国际影视传媒 planets. One in particular is called Kepler-186f, which was discovered about seven years ago. The planet is roughly the same mass as the Earth and is close enough to its star liquid water could potentially exist at the surface.

A chart showing the differences between planets, brown dwarfs and proper stars. Because brown dwarfs are closer to planets in temperature and mass, scientists are studying them to infer what potential weather on exoplanets could be. screenshot courtesy of Aurora Research Institute
A chart showing the differences between planets, brown dwarfs and proper stars. Because brown dwarfs are closer to planets in temperature and mass, scientists are studying them to infer what potential weather on exoplanets could be. screenshot courtesy of Aurora Research Institute

While Metchev notes itSA国际影视传媒檚 unlikely astronomers will be able to see an exoplanet directly for at least a century, that hasnSA国际影视传媒檛 stopped them from estimating what a potential alien world would be like. If there was photosynthesizing life like plants on Kepler-186f, they would likely be mainly red, because the dim light from the nearby star would cast different wavelengths on the planet.

SA国际影视传媒淭he host star itself is dimmer and redder than our own sun so the vegetation would have actually adapted to the red light coming from the star,SA国际影视传媒 he said. SA国际影视传媒淪o the motto for this particular planet is where the grass is always redder on the other side.SA国际影视传媒

Brown Dwarfs light the way

Instead, to develop hypotheses on what conditions on the far-away planets could be like, MentchevSA国际影视传媒檚 team are looking to their larger cousins. Brown Dwarfs are in effect failed stars SA国际影视传媒 massive objects that build up like stars but do not have enough mass to maintain fusion reactions. Consequentially, they behave in a similar manner to large gas giants SA国际影视传媒 many are roughly the same size as Jupiter.

Jupiter at visible and infrared light. Bright spots on the right side show where the hotter, deeper weather systems exist under the surface. screenshot courtesy of Aurora Research Institute
Jupiter at visible and infrared light. Bright spots on the right side show where the hotter, deeper weather systems exist under the surface. screenshot courtesy of Aurora Research Institute

 



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