Home » Technology » For the first time … the heart of a car planet was detected outside the solar system

For the first time … the heart of a car planet was detected outside the solar system

Purchaser And Saturn, but it appears that it has lost its gaseous atmosphere, or that it has failed to form a gaseous atmosphere.

The nucleus planet is known as TOI 849 b and is located about 730 light-years away and orbits around a star similar to the sun.

The TOI 849b planet was first found by the agency’s transient external survey satellite NASA, Which monitors planets by searching for the dim brightness of planets as they move in front of their stars.

The planet was also analyzed by the European Southern Observatory “Harps”, which uses the Doppler effect to measure Exoplanets By looking for the variation in brightness that occurs when the planets are going to become closer or farther from the planet Earth.

According to astronomers, the nucleus planet is very close to its star and is located in an area called the “Neptune desert”, which is known as the region near the stars and there are seldom planets the size of Neptune, which explains the extreme conditions of the planet.

For this planet, one year on its surface takes about 18 hours, while its surface temperature is about 1500 degrees Celsius.

“The planet is very oddly close to its star given its size,” said David Armstrong of Warwick University, lead author of the study. “In other words, planets of this size cannot be seen in these short astronomical orbits close to the stars.”

After making detailed measurements, astronomers found that the nucleus planet TOI 849b was forty times heavier than Earth, but it was 3.4 times the size of it.

This means that the planet’s density comes from that the majority of its composition is mostly iron, rocks and water, with only small amounts of Hydrogen And helium.

“The fact that we do not see these gases on TOI 849b means that it is just the nucleus of a planet,” said Dr. Armstrong.

He added: “One way or another, the TOI 849 b planet was either a gigantic gas planet or it failed to turn into a gaseous planet, but it proves the existence of the planetary nucleus in space and can be found.”

He pointed out that the planet TOI 849b provided an opportunity to look at the nucleus of a planet in a way that could not be done in Our solar system.

He added: “There are still big and open questions about the nature of the nucleus of Jupiter. These exotic planets outside our solar system give us a window to know how the planets are formed that there is no way yet to explore them.

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The discovered planet is roughly the size of Neptune, and this giant planet is believed to be a gaseous planet like a planet Purchaser And Saturn, but it appears that it has lost its gaseous atmosphere, or that it has failed to form a gaseous atmosphere.

The nucleus planet is known as TOI 849 b and is located about 730 light-years away and orbits around a star similar to the sun.

The TOI 849b planet was first found by the agency’s transient external survey satellite NASA, Which monitors planets by searching for the dim brightness of planets as they move in front of their stars.

The planet was also analyzed by the European Southern Observatory “Harps”, which uses the Doppler effect to measure Exoplanets By looking for the variation in brightness that occurs when the planets are going to become closer or farther from the planet Earth.

According to astronomers, the nucleus planet is very close to its star and is located in an area called the “Neptune desert”, which is known as the region near the stars and there are seldom planets the size of Neptune, which explains the extreme conditions of the planet.

For this planet, one year on its surface takes about 18 hours, while its surface temperature is about 1500 degrees Celsius.

“The planet is very oddly close to its star given its size,” said David Armstrong of Warwick University, lead author of the study. “In other words, planets of this size cannot be seen in these short astronomical orbits close to the stars.”

After making detailed measurements, astronomers found that the nucleus planet TOI 849b was forty times heavier than Earth, but it was 3.4 times the size of it.

This means that the planet’s density comes from that the majority of its composition is mostly iron, rocks and water, with only small amounts of Hydrogen And helium.

“The fact that we do not see these gases on TOI 849b means that it is just the nucleus of a planet,” said Dr. Armstrong.

He added: “One way or another, the TOI 849 b planet was either a gigantic gas planet or it failed to turn into a gaseous planet, but it proves the existence of the planetary nucleus in space and can be found.”

He pointed out that the planet TOI 849b provided an opportunity to look at the nucleus of a planet in a way that could not be done in Our solar system.

He added: “There are still big and open questions about the nature of the nucleus of Jupiter, as these strange planets outside our solar system give us a window to know how the planets are formed that there is no way so far to explore them.

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