transit photometry tagged posts

Could the ESA’s PLATO Mission find Earth 2.0?

Artist’s impression of the ESA’s PLATO mission. Credit: ESA/ATG medialab

Currently, 5,788 exoplanets have been confirmed in 4,326 star systems, while thousands more candidates await confirmation. So far, the vast majority of these planets have been gas giants (3,826) or Super-Earths (1,735), while only 210 have been “Earth-like”—meaning rocky planets similar in size and mass to Earth.

What’s more, the majority of these planets have been discovered orbiting within M-type (red dwarf) star systems, while only a few have been found orbiting sun-like stars. Nevertheless, no Earth-like planets orbiting within a sun-like star’s habitable zone (HZ) have been discovered so far.

This is largely due to the limitations of existing observatories, which have been unable to resolve Earth-size...

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Scientists detect Comets Outside our Solar System

An artist’s conception of a view from within the Exocomet system KIC 3542116. Credit: Danielle Futselaar

An artist’s conception of a view from within the Exocomet system KIC 3542116. Credit: Danielle Futselaar

Tails of comets seen streaking past a distant star. Scientists from MIT and other institutions, working closely with amateur astronomers, have spotted the dusty tails of 6 exocomets – comets outside our solar system – orbiting a faint star 800 light years from Earth. These cosmic balls of ice and dust, about the size of Halley’s Comet and traveled about 100,000 miles per hour before they ultimately vaporized, are some of the smallest objects yet found outside our own solar system.

The discovery marks the first time that an object as small as a comet has been detected using transit photometry, a technique by which astronomers observe a star’s light for telltale dips in intensity...

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Finding new Worlds with a Play of Light and Shadow

Finding new worlds with a play of light and shadow

The most successful technique for finding planets beyond our solar system so far is transit photometry, which measures changes in a star’s brightness caused by a mini-eclipse. When a planet crosses in front of its star along our line of sight, it blocks some of the star’s light. If the dimming lasts for a set amount of time and occurs at regular intervals, it likely means an exoplanet is passing in front of, or transiting, the star once every orbital period.

NASA’s Kepler Space Telescope has used this technique to become the most successful planet-hunting spacecraft to date, with more than a thousand established discoveries and many more awaiting confirmation...

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