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• You are proficient in English, level C1 or C2 (mandatory)
• You have a technical background (desirable)
• You are very organized
• You have experience in the field of communication and public relations (desirable)
• Punctuality and prioritization are your friends
• Writing in English and Romanian, various lengths
Type of job
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- Please write a summary of 100 words in Romanian for the following news item:
A giant planet has been found orbiting an ultracool dwarf star — the largest planet compared to its star ever found — leaving scientists baffled at how the duo could have formed.
The planet NGTS-1b is situated 600 light-years from our solar system, according to a statement from the University of Warwick, and it is a gas giant about the size of Jupiter. Its star, on the other hand, is just half the mass and radius of the sun. The planet orbits its star at 3 percent the distance from the Earth to the sun, and it whips around a full orbit every Earth days.
An international collaboration of researchers found the planet using the Next-Generation Transit Survey, an array of 12 telescopes at the Paranal Observatory in northern Chile that searches for a telltale dimming in distant stars that would indicate planets passing by.
The system's star is a small, dim M-dwarf, which is the most common type of star in the sky. Red dwarfs burn their fuel much more slowly than sun-like stars, so they can have lifetimes of trillions of years. According to the new work, this is the third time a gas giant has been seen orbiting an M-dwarf — but this planet is by far the largest.
While it can be tricky enough just to spot planets orbiting M-dwarfs, researchers are much more used to seeing M-dwarfs orbited by rocky planets, according to a statement from the Royal Astronomical Society.
To find NGTS-1b, the Next-Generation Transit Survey monitored certain spots in the sky for months with red-sensitive cameras to catch any changes in brightness to stars in its field of view, according to the statement from the University of Warwick. Researchers saw the particular M-dwarf dipping in brightness every days, suggesting it had a planetary companion. Then, they confirmed the planet's gargantuan size by measuring its radial velocity — how much the star "wobbles" during each orbit from its companion's gravitational pull.