By MICHELLE GILLIAN and CHRIS MARTIN, Associated Press A rare, early detection of a celestial event can provide clues about how our universe began and how life evolved.
Astronomers are searching for signals in the sky that could help explain how the universe formed, why stars formed, and why galaxies form.
Astronomers have a good idea how our solar system began with the birth of our Sun, but we don’t know what it looked like when it was born.
A new study suggests that a star may have been born when the universe was only about 1.5 billion years old.
The study, led by astronomers at the University of California, Santa Cruz, and the University in Berlin, has found a signal from a distant star that has yet to be discovered.
Astrophysicist Stephen Bae of the UC Santa Cruz Institute of Astronomy and the German Aerospace Center said the signal is “quite promising.”
The study was published Friday in the journal Nature Astronomy.
The new star, called Deneb 917, has been known since 2014 by the nickname Draco.
It is about 40 light-years from Earth in the constellation Draco.
The researchers believe it’s the closest object in the Crab Nebula, a group of galaxies that contain some of the oldest stars in the universe.
The Crab Nebula is thought to have formed when the Milky Way, a massive group of stars and gas, collided with the smaller group of larger galaxies.
The Crab Nebula has been identified in a variety of ways.
The team looked for infrared emission from the star and the gravitational effects of the Crab, a star about twice as massive as our Sun.
The results are consistent with what the Crab emits when it’s orbiting.
The light from the Crab is visible to the naked eye, but the infrared emissions from Denep 917 are invisible to the human eye.
The infrared emission is a type of radiation that is emitted by a star.
This is called optical emission, and it’s what the infrared camera on the Hubble Space Telescope can see.
This means the astronomers were able to see a faint emission from Denesb 918.
The astronomers think that the infrared emission was caused by the Crab’s orbital motion around the star, as well as the intense gravitational pull of the star.
Astroscopic observations also revealed that Denev 917 has two stars.
The first, known as a red giant, is about a billion times the mass of the Sun.
It was found by a Japanese observatory and astronomers are searching it for more information.
The second, known simply as a brown dwarf, is an intermediate red giant.
Its name is a play on the word brown.
The brown dwarf is the smallest star in the galaxy known.
Scientists think the two stars formed when a massive star exploded when Deneva 917 passed between the two planets.
The two stars are known as Denebos, because they’re part of a family of brown dwarfs.
Astronomer Peter Zemmour of the University at Birmingham in the UK is the first author of the paper.
It says the new star has a mass of about 5,000 times the sun’s.
It’s very unusual that this is found in the first place, said the study’s lead author, physicist Tiziana D’Onofrio of the Institut d’Astrophysics de Paris in France.
She was not involved in the study.
This is the second time the Crab has been spotted.
The star was first seen in the early 2000s, and astronomers think it’s a member of a class of young, hot, gas-giant stars that formed as they cooled.
They were so hot that they exploded as a giant star, which is why they’re so easy to spot.
The stars in Denebs 917 were discovered as part of the search for a previously unknown type of supernova remnant called a supernova.
A supernova is a supermassive black hole in the center of a galaxy that creates an explosion that destroys everything in its path.
A typical supernova produces about 100 million suns and billions of stars.
Astrologers estimate that Denes 917 is about 25 million light-year away from Earth.
The galaxy is in the southern constellation Aquarius, and is about 60,000 light-seconds from Earth’s surface.