Astronomy

High-Speed Video Cameras Capture Shooting Stars

December 17, 2019, 8:30 AM HST
* Updated December 17, 9:56 AM
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A new monitoring system was installed on existing rooftop buildings on Maunakea and Haleakalā, which allows astronomers to detect meteors through a different lens.

The detectors, a high-speed video device, is part of an expanding network of identical cameras in the Automated Meteor Observations System. They are programmed to capture shooting stars, or non-threatening meteors.

“Shooting stars” are miniature bits of space debris, which are relics of the early solar system, shining as they burn up in the atmosphere 60 miles above someone standing on Earth at 15 times the muzzle speed of high-powered rifles.

According to astronomers, the tiny meteors hold clues to the formation and continuing development of the solar system. Technically, they are called “meteors,” and are so numerous that they increase the mass of the Earth by about 20,000 tons per year.

“The opportunity to install AMOS systems on Maunakea and Haleakalā, two of the finest astronomical sites in the world, will provide us data to track meteors across the sky and determine their composition,” explained Peter Veres, an AMOS co-investigator at the Center for Astrophysics at Harvard University, and formerly at the University of Hawaiʻi Institute for Astronomy (IfA).

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AMOS uses fish-eye lenses to continuously take a video of the entire sky all night long. The advantage of having systems on both mountaintops is that meteors imaged by two cameras can be divided to determine their true path through the sky. The high-speed video images allow the researchers to determine a meteor’s speed at each point along its trajectory, so they can compute the deceleration of the debris due to air friction. After accounting for the atmosphere’s effect on the meteor they can project the particle’s path backwards in time to determine the meteoroidʻs original orbit around the Sun, before it encountered Earth.

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About half of all meteors come from “showers” of dust ejected long ago by an asteroid or comet, and planetary scientists sometimes know exactly which comet or asteroid is associated with a particular shower.

The AMOS system on Maunakea acquires a range of the brightest meteors during their fiery death plunge, that are then used to determine the types of atoms that the meteors contained.

“Combining the information about what a meteor is linked to allows us to determine the makeup of many comets and asteroids without the cost of sending spacecraft to each one,” said Robert Jedicke, a faculty member at IfA, and a collaborator on the AMOS project.

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The long-term goal of the project is to determine how the elements are distributed throughout our solar system. The detailed information provided from the meteors can be combined with information from ground- and space-based telescopes and spacecraft missions to build a comprehensive picture of how the solar system formed and continues to evolve.

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