Proxima b is promising but don’t start looking for E.T.
Scientists have confirmed the existence of a rocky—and possibly wet—planet orbiting Proxima Centauri, the closest star to our sun. Dubbed Proxima b, the planet lies within the “habitable zone” of its star, meaning the planet’s surface could be warm enough, but not too warm, to support liquid water and thus be amenable for life.
Astronomers found Proxima b by analyzing Doppler data and other measurements from telescopes around the world, chiefly ESO telescopes mounted at the La Silla Observatory in Chile. The results of the study were first reported in the journal Nature.
Located 4.2 light years away from Earth, Proxima b is notably the closest terrestrial planet outside our solar system ever found. While that might still seem like a haul, scientists believe the potential exists for robotic exploration of the world in the coming centuries. Researchers have already provided a snapshot of the planet, which likely [revolves around] its star every 11.2 days; is about 1.3 the mass of Earth; and is possibly tidally locked, meaning one half of the planet is forever bathed in light and radiation, while the outward-facing side remains dark.
Sarah Hörst, an assistant professor in the earth and planetary sciences department at Johns Hopkins University, offers some perspective on what some are calling “an astronomy dream come true” and Earth 2.0.
I’ll admit, I was a little geeked out when I heard the news. An Earth-like world, potentially habitable, and so relatively close. What was your initial reaction to the new exoplanet, and is this level of excitement justified?
A lot of people have mentioned being really excited about the news, which makes me exceedingly happy. Ultimately, I really want the public to understand what we do and to be inspired to look up and think about worlds far beyond our own. For me, every new world that we learn about is another piece to the “how worlds work” puzzle that we are trying to put together, so I am always excited when we learn about other worlds.
I noticed you playfully tweeted out a “PSA” that planets in the so-called habitable zone are not necessarily habitable. And just being Earth-sized doesn’t mean grab your beach ball, we’re headed for sun and fun on Proxima b. Can you expand on your thoughts on why being in the habitable zone doesn’t essentially mean E.T. is walking on the surface?
It is important to remember that the habitable zone refers only to the possibility of liquid water on the surfaces of planets located in that zone. Whether or not those planets actually have liquid water depends on a number of factors, including presence and composition of an atmosphere—which affects surface temperature and pressure—how much water (if any) the planet has, etc.
Venus and Mars are on the edges of the habitable zone in our solar system and liquid water isn’t stable on either of their surfaces today. So being in the habitable zone doesn’t even mean a planet will have liquid water on its surface. If it does have liquid water, that still doesn’t mean it will have life, because life, as far as we understand, requires a number of other things, like a source of energy and organic molecules.
Your expertise is in planetary atmospheres. Do we know yet if Proxima b has an atmosphere or not, and if so, what it might be like?
We don’t know yet if Proxima b has an atmosphere. It is also kind of difficult to speculate what it might be like. Within our own solar system we see a diversity of planetary atmospheres, and we are still working to understand what determined which worlds have atmospheres, where those atmospheres came from, and what they are made of. This is one of the many reasons why exoplanets, including Proxima b, are so interesting for those of us that study the solar system. They are adding numerous more data points that we can use in our quest to understand how planets work.
We should be able to find out if Proxima b has an atmosphere using the James Webb Space Telescope, which launches in 2018 and will be operated from the Space Telescope Science Institute, located on our Homewood campus. And by looking at how the amount of heat [the planet] emits varies as a function of the position in its orbit. If an atmosphere were present it would redistribute heat.
I have to admit, my first reaction was somewhat dubious: How could there be an Earth-like world located literally around the nearest star outside our solar system? How did we not spot this exoplanet before, as you’d think this would be the first place we’d look?
Proxima b is around a type of star called an M dwarf, which is a very active star. Stellar activity complicates analysis of data when looking for planets. People have been looking for a planet around Proxima Centauri for a while and their persistence and improvements in data processing finally paid off. It is much more difficult to rule out a false positive for an active star, so the burden of proof is higher for a star like Proxima Centauri.
I’ve read the planet is close to its star, perhaps as close or closer than Mercury is to our sun. But Proxima Centauri is cooler and fainter than our sun. Still, what would be the impact of being so close?
The location of the habitable zone is determined by the amount of energy coming from the star, so for stars like Proxima Centauri, the habitable zone is closer to the star than it is in our solar system.
The closer a planet gets to its star, the more likely it is to be tidally locked, which means that the same side of the planet always faces the star. Our moon is tidally locked to Earth, which is why we can only see one side from Earth. Planets that are tidally locked can end up with very large temperature differences between the side of the planet that faces the star (hot!) and the side that faces away from the star (cold!), especially if they don’t have an atmosphere to redistribute heat. Tidally locked planets may be less favorable for life, but that is something that we are still trying to understand. Having only one example of life makes it a bit difficult to know where life can exist.
How important is it that we learn more about the formation of this planet and its star?
Our solar system has one star, with a small—in the grand scheme of things—number of worlds orbiting it that all formed from the same reservoir of starting material. It amounts to one data point about how planetary systems work.
To really understand the fundamental physical and chemical processes that underlie the world we observe, we usually need lots of points of data that cover the range of conditions that