Thursday, August 25

A New Planetary Neighbor

It appears we overlooked our nearest neighboring star, the red dwarf Proxima Centauri, as a potential host of planets. Until now.

A new paper published in Nature tells the story:
At a distance of 1.295 parsecs, the red dwarf Proxima Centauri (α Centauri C, GL 551, HIP 70890 or simply Proxima) is the Sun’s closest stellar neighbour and one of the best-studied low-mass stars. It has an effective temperature of only around 3,050 kelvin, a luminosity of 0.15 per cent of that of the Sun, a measured radius of 14 per cent of the radius of the Sun and a mass of about 12 per cent of the mass of the Sun. Although Proxima is considered a moderately active star, its rotation period is about 83 days and its quiescent activity levels and X-ray luminosity are comparable to those of the Sun. Here we report observations that reveal the presence of a small planet with a minimum mass of about 1.3 Earth masses orbiting Proxima with a period of approximately 11.2 days at a semi-major-axis distance of around 0.05 astronomical units. Its equilibrium temperature is within the range where water could be liquid on its surface.
How did we miss it? It seems we have been more interested in stars like our own sun, but attitudes are changing. 

Now that the speculation has started, we can expect much more attention regarding his new world.

Maybe this would have been as easier trip for the voyagers in Kim Stanley Robinson's novel Aurora rather than Tau Ceti, which is about three times more distant. It seems to be another case of reality trumping fiction.