In 2015, a star called KIC 8462852 caused quite a stir in and beyond the astronomy community due to a series of rapid, unexplained dimming events seen while it was being monitored by NASA’s Kepler Space Telescope. And the star has continued to foil scientists’ efforts to understand it ever since.
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| An inconspicuous star—KIC 8462852—harbors a great mystery. This ASAS-SN image is just a small portion of the sky, but shows how Tabby's star is one of millions [Credit: Benjamin Shappee] |
Speculation to account for KIC 8462852’s dips in brightness has ranged from it having swallowed a nearby planet to an unusually large group of comets orbiting the star to an alien megastructure.
In general, stars can appear to dim because a solid object like a planet or a cloud of dust and gas passes between it and the observer, eclipsing and effectively dimming its brightness for a time. But even before this evidence of two periods of increased brightness in the star’s past, the erratic dimming periods seen in KIC 8462852 were unlike anything astronomers had previously observed.
Last year, Simon and Ben Montet (then at Caltech, now at University of Chicago), who is also a co-author on this current study, found that from 2009 to 2012, KIC 8462852 dimmed by almost 1 percent. Its brightness then dropped by an extraordinary 2 percent over just six months, remaining at about that level for the final six months of Kepler observations.
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| This illustration depicts a hypothetical uneven ring of dust orbiting KIC 8462852, also known as Boyajian's Star or Tabby's Star. Astronomers have found the dimming of the star over long periods appears to be weaker at longer infrared wavelengths of light and stronger at shorter ultraviolet wavelengths. Such reddening is characteristic of dust particles and inconsistent with more fanciful "alien megastructure" concepts, which would evenly dim all wavelengths of light. By studying observations from NASA's Spitzer and Swift telescopes, as well as the Belgian AstroLAB IRIS observatory, the researchers have been able to better constrain the size of the dust particles. This places them within the range found in dust disks orbiting stars, and larger than the particles typically found in interstellar dust. The system is portrayed with a couple of comets, consistent with previous studies that have found evidence for cometary activity within the system [Credit: NASA/JPL-Caltech] |
They found that the star has continued to dim since 2015 and is now 1.5 percent fainter than it was in February of that year. What’s more, they showed that in addition to the dimming the star has experienced from 2009 to 2013 and 2015 to now, it underwent two periods of brightening.
“Up until this work, we had thought that the star’s changes in brightness were only occurring in one direction—dimming,” Simon explained. “The realization that the star sometimes gets brighter in addition to periods of dimming is incompatible with most hypotheses to explain its weird behavior.”
“An important next step will be to determine how the color of the star changes with time, especially during its brief dips in brightness,” added Shappee. “That information would help narrow down the possible explanations for why this star is doing such strange things.”
For example, if the dimming was caused by dust obscuring the star from us, then it would appear to get redder as it dimmed. But if large objects were blocking the star’s light, then no color change would be seen.
“We haven’t solved the mystery yet,” Simon concluded. “But understanding the star's long-term changes is a key piece of the puzzle."
The study is published in The Astrophysical Journal.
Source: Carnegie Institution for Science [October 04, 2017]
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