Universe Today
In August of 2016, the European Southern Observatory announced that the nearest star to our own - Proxima Centauri -
had an exoplanet
. Since that time, considerable attention has been focused on this world (Proxima b) in the hopes of determining just how "Earth-like" it really is. Despite all indications of it being
terrestrial
and similar in mass to Earth, there are some lingering doubts about its ability to support life.
This is largely due to the fact that Proxima b orbits a red dwarf. Typically, these low mass, low temperature, slow fusion stars are not known for being as bright and warm as our Sun. However,
a new study
produced by researchers at the
Harvard Smithsonian Center for Astrophysics
(CfA) has indicated that Proxima Centauri might be more like our star than we thought.
For instance, our Sun has what is known as a "
Solar Cycle
", an 11-year period in which it experiences
changes in the levels of radiation it emits. This cycle is driven by changes in the Sun's own magnetic field, and corresponds to the appearance of Sunspots on its surface. During a "solar minimum", the Sun's surface is clear of spots, while at a solar maximum, one hundred sunspots can appear on an area the size of 1% the Sun's surface area.
[caption id="attachment_101620" align="aligncenter" width="580"]
Composite of 25 separate images spanning the period of April 16, 2012, to April 15, 2013, revealing active regions during this part of the Solar Cycle.
Credit: NASA/SDO/AIA/S. Wiessinger
[/caption]
For the sake of their research, the Harvard Smithsonian team examined Proxima Centauri over the course of several years to see if it too had a cycle. As they explain in their research paper, titled "
Optical, UV, and X-Ray Evidence for a 7-Year Stellar Cycle in Proxima Centauri
" they relied on several years worth optical, UV, and X-ray observations made of the star.
This included 15 years of visual data and 3 years of infrared data from the
All Sky Automated Survey
(ASAS), 4 years of x-ray and UV data from the
Swift x-ray telescope
(XRT), and 22 years worth of x-ray observations taken by the
Advanced Satellite for Cosmology and Astrophysics
(ASCA), the
XXM-Newton
mission and the
Chandra X-ray Observatory
.
What they found was that Proxima Centauri does indeed have a cycle that involves changes in its minimum and maximum amount of emitting radiation, which corresponds to "starspots" on its surface. As Dr. Wargelin told Universe Today via email:
In essence, Proxima Centauri has its own cycle, but one that is a lot more dramatic than our Sun's. Besides lasting 7 years from peak to peak, it involves spots covering over 20% of its surface at one time. These spots are apparently much bigger than the ones we regularly observe on our Sun as well.
[caption id="attachment_24790" align="aligncenter" width="576"]
An X-Ray image of Proxima Centauri. Credit: Chandra/Harvard/NASA
[/caption]
This was surprising, given that Proxima's interior is very different from our Sun's. Because of its low mass, the interior of Proxima Centauri is convective, where material in the core is transferred outward. In contrast, only the outer layer of our Sun undergoes convection while the core remains relatively still. This means that, unlike our Sun, energy is transferred to the surface through physical movement, and not radiative processes.
While these findings cannot tell us anything directly about whether or not Proxima b might be habitable, the existence of this solar cycle is an interesting find that might be leading in that general direction. As Dr. Wargelin explained:
As always, further observations and research will be necessary before we can fully understand Proxima Centauri, and whether or not any planets that orbit it could support life. But then again, we've only known about Proxima b for a short time, and the rate at which we are learning new things about it is quite impressive!
Further Reading: CfA
,
arXiv
