Photobombing exoplanets might thwart search for extraterrestrial life
It's frustrating when a stranger photobombs your family photo when you're on vacation. But when an exoplanet photobombs a space telescope's image of another exoplanet, it could actually ruin a scientist's research.
Yes, planetary photobombing is a thing — sort of. For those who don't know what photobomb means, Merriam-Webster defines it as "to move into the frame of a photograph as it is being taken as a joke or prank." The catch is that exoplanets aren't intentionally ruining a photograph, but they might inadvertently do so.
A new study led by Prabal Saxena, a scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, indicates that a space telescope's image of a distant exoplanet (that is, a planet outside our solar system) might be contaminated by the light from another nearby exoplanet. That could potentially create errors when analyzing data — specifically the light spectra that could indicate an exoplanet's chemical composition.
"If you looked at Earth sitting next to Mars or Venus from a distant vantage point, then depending on when you observed them, you might think they're both the same object," Saxena said in a statement(opens in new tab).
Because space telescopes have to "see" across extremely vast distances, light diffraction could likely cause two exoplanets to visually merge. That causes problems when scientists are attempting to analyze the spectra of an exoplanet in search of biosignatures, or signs of life. Cross-contamination from a different object could completely confuse the results.
Thus Saxena's team suggested several methods that could mitigate planetary photobombing, from using multiple telescopes to examine the same area to using a single telescope to observe the exoplanets over an extended period of time, which might help distinguish the object from the photobomber as they move in their orbits.
The scientists, however, say that more research is required to solve the problem effectively.
The team's research was published in the Astrophysical Journal Letters(opens in new tab) on Aug. 11.
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