Could the Milky Way have 9 planets after all? Astronomers may have confirmed possible existence.
Our solar system may have a ninth planet after all, researchers say.
The possibility that an additional planet may be hidden far into the solar system was touted more than a century ago. But astronomers may have found new evidence that points to a celestial body that could be a possible candidate as "Planet Nine," according to a new paper, which has been accepted for publication in the Publications of the Astronomical Society of Australia but not yet peer-reviewed.
MORE: Exoplanet discovered in 2020 has the coldest temperatures ever measured, scientists say
The hidden candidate is likely the size of Neptune and is so far away that it could take between 10,000 and 20,000 years to orbit the sun, according to the paper.
Two deep infrared surveys taken 23 years apart measured the object's orbital motion. In 1983, the Infrared Astronomy Satellite surveyed the universe for a year. In 2006, the Japanese Aerospace Exploration Agency launched the infrared satellite AKARI, which was active until 2011.
Researchers at the University in Taiwan compared objects that were observed in the IRAS database with the data obtained by AKARI to see if there were any movements within that time frame.
The candidate for Planet Nine displayed a tiny amount of movement, which could mean it advanced further in its orbit around the sun.
Some of the strongest evidence that points to the existence of a planet within the outskirts of the solar system is the activity within the Kuiper Belt, an unusual clustering of icy bodies -- including comets and dwarf planets -- which stretches from Neptune and outward toward interstellar space.
MORE: Several planets found orbiting star less than 6 light-years away
Six known objects in the Kuiper Belt have elliptical orbits pointing in the same direction. In addition, objects from the Kuiper Belt orbit in the opposite direction from everything else in the solar system, according to NASA. This could be the result of a gravitational pull from a nearby planet, the researchers said.
Moreover, the object reflects just a faint amount of sunlight, furthering the likelihood that it is, indeed, a planet, according to the study.
The International Astronomical Union downgraded Pluto's classification to a dwarf planet in 2006, mainly because other objects might cross its orbit. Pluto was previously considered to be the ninth planet in our solar system, but the new definition of a planet requires the celestial body to have enough gravity to clear its orbital path from other bodies.
MORE: Binary star system found near the Milky Way's black hole: An 'amazing' discovery, astrophysicists say
There are currently several lines of observational evidence pointing to the existence of Planet Nine, according to NASA.
The surveys did not provide enough data to determine the full orbit of the planetary candidate, meaning more observations will be needed, the researchers said.
Could the Milky Way have 9 planets after all? Astronomers may have confirmed possible existence. originally appeared on abcnews.go.com
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'NSF-DOE Rubin Observatory will capture more information about our universe than all optical telescopes throughout history combined,' said National Science Foundation Chief of Staff Brian Stone, who is currently performing the duties of the NSF director (as the position is currently vacant). Among the observatory's initial accomplishments was the discovery of 2,104 asteroids, including seven near-Earth asteroids, that have never been seen before in our solar system. None of the newly found near-Earth asteroids pose a risk to our planet, according to scientists at the observatory. Imagery of the asteroids is expected to be shared later Monday. While ground- and space-based telescopes spot about 20,000 asteroids each year, Rubin Observatory is expected to uncover millions of the space rocks within its first two years, according to the National Science Foundation. The telescope is also considered the most effective way to spot any interstellar comets or asteroids that may travel through our solar system. The observatory's mirror design, sensitive camera and telescope speed are all the first of its kind, enabling Rubin to spot tiny, faint objects such as asteroids. The observatory will also constantly take thousands of images every night, cataloging changes in brightness to reveal otherwise hidden space rocks like near-Earth asteroids that could be on a collision course with our planet, according to the foundation. A sneak peek shared Monday includes a video made from over 1,100 images captured by the observatory that begins with a detailed look at two galaxies. The video then zooms out to showcase about 10 million galaxies spotted by the camera's wide view — roughly 0.05% of the 20 billion galaxies Rubin will observe over 10 years. The observatory team also released a mosaic of the Trifid and Lagoon nebulae, which are star-forming regions that resemble clouds located in the Sagittarius constellation. The mosaic, made up of 678 separate images taken over just seven hours, captured faint and previously invisible details such as clouds of gas and dust in the nebulae, which are several thousand light-years away from Earth. The initial images were selected to showcase the telescope's enormous field of view, which enables detailed glimpses of interacting galaxies as well as broad views of millions of galaxies, said Dr. Yusra AlSayyad, deputy associate director of the data management subsystem for the Rubin Observatory. 'It has such a wide field of view and such a rapid cadence that you do have that movielike aspect to the night sky,' said Dr. Sandrine Thomas, telescope project scientist for the Rubin Observatory. The observatory, located in the Andes on the top of Cerro Pachón in Chile, is nearly complete after about two decades of work. The facility is set to achieve 'first light,' or make the first scientific observations of the Southern Hemisphere's sky using its 8.4-meter (27.5-foot) Simonyi Survey Telescope, on July 4. The telescope's location in the Southern Hemisphere allows for a great view of the Milky Way's galactic center, said Edward Ajhar, Rubin Observatory's program officer. The region in central Chile has also been home to other ground-based observatories and is favored for astronomical observations because it affords dry air and dark skies. The observatory's main objective is the Legacy Survey of Space and Time, an ultrawide and ultra-high-definition movie of the universe made by scanning the entire sky every few nights over 10 years to capture a time-lapse compilation of whizzing asteroids and comets, exploding stars, and distant galaxies as they change. 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The telescope's namesake, considered to be one of the most influential women astronomers, provided some of the first evidence that dark matter existed. In Rubin's honor, the telescope is expected to continue her pioneering work. 'Through this remarkable scientific facility, we will explore many cosmic mysteries, including the dark matter and dark energy that permeate the universe,' Stone said. Dark matter is an enigmatic substance that shapes the cosmos, while dark energy is a force that accelerates the expansion rate of the universe, according to NASA. Though they are thought to make up most of the cosmos, both are impossible to directly observe but can be detected due to their gravitational effects. 'Rubin has enormous potential to help us learn what dark energy really is and how the universe's expansion is accelerating here, too,' Roodman said. 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'NSF-DOE Rubin Observatory will capture more information about our universe than all optical telescopes throughout history combined,' said National Science Foundation Chief of Staff Brian Stone, who is currently performing the duties of the NSF director (as the position is currently vacant). Among the observatory's initial accomplishments was the discovery of 2,104 asteroids, including seven near-Earth asteroids, that have never been seen before in our solar system. None of the newly found near-Earth asteroids pose a risk to our planet, according to scientists at the observatory. Imagery of the asteroids is expected to be shared later Monday. While ground- and space-based telescopes spot about 20,000 asteroids each year, Rubin Observatory is expected to uncover millions of the space rocks within its first two years, according to the National Science Foundation. The telescope is also considered the most effective way to spot any interstellar comets or asteroids that may travel through our solar system. The observatory's mirror design, sensitive camera and telescope speed are all the first of its kind, enabling Rubin to spot tiny, faint objects such as asteroids. The observatory will also constantly take thousands of images every night, cataloging changes in brightness to reveal otherwise hidden space rocks like near-Earth asteroids that could be on a collision course with our planet, according to the foundation. A sneak peek shared Monday includes a video made from over 1,100 images captured by the observatory that begins with a detailed look at two galaxies. The video then zooms out to showcase about 10 million galaxies spotted by the camera's wide view — roughly 0.05% of the 20 billion galaxies Rubin will observe over 10 years. The observatory team also released a mosaic of the Trifid and Lagoon nebulae, which are star-forming regions that resemble clouds located in the Sagittarius constellation. The mosaic, made up of 678 separate images taken over just seven hours, captured faint and previously invisible details such as clouds of gas and dust in the nebulae, which are several thousand light-years away from Earth. The initial images were selected to showcase the telescope's enormous field of view, which enables detailed glimpses of interacting galaxies as well as broad views of millions of galaxies, said Dr. Yusra AlSayyad, deputy associate director of the data management subsystem for the Rubin Observatory. 'It has such a wide field of view and such a rapid cadence that you do have that movielike aspect to the night sky,' said Dr. Sandrine Thomas, telescope project scientist for the Rubin Observatory. The observatory, located in the Andes on the top of Cerro Pachón in Chile, is nearly complete after about two decades of work. The facility is set to achieve 'first light,' or make the first scientific observations of the Southern Hemisphere's sky using its 8.4-meter (27.5-foot) Simonyi Survey Telescope, on July 4. The telescope's location in the Southern Hemisphere allows for a great view of the Milky Way's galactic center, said Edward Ajhar, Rubin Observatory's program officer. The region in central Chile has also been home to other ground-based observatories and is favored for astronomical observations because it affords dry air and dark skies. The observatory's main objective is the Legacy Survey of Space and Time, an ultrawide and ultra-high-definition movie of the universe made by scanning the entire sky every few nights over 10 years to capture a time-lapse compilation of whizzing asteroids and comets, exploding stars, and distant galaxies as they change. The survey is expected to begin between four to seven months after first light. '(Rubin) will enable us to explore galaxies, stars in the Milky Way, objects in the solar system, and all in a truly new way. Since we take images of the night sky so quickly and so often, (it) will detect millions of changing objects literally every night,' said Dr. Aaron Roodman, professor of particle physics and astrophysics at Stanford University's SLAC National Accelerator Laboratory in California. Roodman was responsible for the assembly and testing of Rubin Observatory's camera. Rubin's capabilities to spot interesting phenomena will also enable it to be a 'discovery machine' that can identify interesting areas of focus for other telescopes, Roodman said. The observatory could also enable the detection of previously unknown types of celestial objects. The telescope's namesake, considered to be one of the most influential women astronomers, provided some of the first evidence that dark matter existed. In Rubin's honor, the telescope is expected to continue her pioneering work. 'Through this remarkable scientific facility, we will explore many cosmic mysteries, including the dark matter and dark energy that permeate the universe,' Stone said. Dark matter is an enigmatic substance that shapes the cosmos, while dark energy is a force that accelerates the expansion rate of the universe, according to NASA. Though they are thought to make up most of the cosmos, both are impossible to directly observe but can be detected due to their gravitational effects. 'Rubin has enormous potential to help us learn what dark energy really is and how the universe's expansion is accelerating here, too,' Roodman said. 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'NSF-DOE Rubin Observatory will capture more information about our universe than all optical telescopes throughout history combined,' said National Science Foundation Chief of Staff Brian Stone, who is currently performing the duties of the NSF director (as the position is currently vacant). Among the observatory's initial accomplishments was the discovery of 2,104 asteroids, including seven near-Earth asteroids, that have never been seen before in our solar system. None of the newly found near-Earth asteroids pose a risk to our planet, according to scientists at the observatory. Imagery of the asteroids is expected to be shared later Monday. While ground- and space-based telescopes spot about 20,000 asteroids each year, Rubin Observatory is expected to uncover millions of the space rocks within its first two years, according to the National Science Foundation. The telescope is also considered the most effective way to spot any interstellar comets or asteroids that may travel through our solar system. The observatory's mirror design, sensitive camera and telescope speed are all the first of its kind, enabling Rubin to spot tiny, faint objects such as asteroids. The observatory will also constantly take thousands of images every night, cataloging changes in brightness to reveal otherwise hidden space rocks like near-Earth asteroids that could be on a collision course with our planet, according to the foundation. A sneak peek shared Monday includes a video made from over 1,100 images captured by the observatory that begins with a detailed look at two galaxies. The video then zooms out to showcase about 10 million galaxies spotted by the camera's wide view — roughly 0.05% of the 20 billion galaxies Rubin will observe over 10 years. The observatory team also released a mosaic of the Trifid and Lagoon nebulae, which are star-forming regions that resemble clouds located in the Sagittarius constellation. The mosaic, made up of 678 separate images taken over just seven hours, captured faint and previously invisible details such as clouds of gas and dust in the nebulae, which are several thousand light-years away from Earth. The initial images were selected to showcase the telescope's enormous field of view, which enables detailed glimpses of interacting galaxies as well as broad views of millions of galaxies, said Dr. Yusra AlSayyad, deputy associate director of the data management subsystem for the Rubin Observatory. 'It has such a wide field of view and such a rapid cadence that you do have that movielike aspect to the night sky,' said Dr. Sandrine Thomas, telescope project scientist for the Rubin Observatory. The observatory, located in the Andes on the top of Cerro Pachón in Chile, is nearly complete after about two decades of work. The facility is set to achieve 'first light,' or make the first scientific observations of the Southern Hemisphere's sky using its 8.4-meter (27.5-foot) Simonyi Survey Telescope, on July 4. The telescope's location in the Southern Hemisphere allows for a great view of the Milky Way's galactic center, said Edward Ajhar, Rubin Observatory's program officer. The region in central Chile has also been home to other ground-based observatories and is favored for astronomical observations because it affords dry air and dark skies. The observatory's main objective is the Legacy Survey of Space and Time, an ultrawide and ultra-high-definition movie of the universe made by scanning the entire sky every few nights over 10 years to capture a time-lapse compilation of whizzing asteroids and comets, exploding stars, and distant galaxies as they change. The survey is expected to begin between four to seven months after first light. '(Rubin) will enable us to explore galaxies, stars in the Milky Way, objects in the solar system, and all in a truly new way. Since we take images of the night sky so quickly and so often, (it) will detect millions of changing objects literally every night,' said Dr. Aaron Roodman, professor of particle physics and astrophysics at Stanford University's SLAC National Accelerator Laboratory in California. Roodman was responsible for the assembly and testing of Rubin Observatory's camera. Rubin's capabilities to spot interesting phenomena will also enable it to be a 'discovery machine' that can identify interesting areas of focus for other telescopes, Roodman said. The observatory could also enable the detection of previously unknown types of celestial objects. The telescope's namesake, considered to be one of the most influential women astronomers, provided some of the first evidence that dark matter existed. In Rubin's honor, the telescope is expected to continue her pioneering work. 'Through this remarkable scientific facility, we will explore many cosmic mysteries, including the dark matter and dark energy that permeate the universe,' Stone said. Dark matter is an enigmatic substance that shapes the cosmos, while dark energy is a force that accelerates the expansion rate of the universe, according to NASA. Though they are thought to make up most of the cosmos, both are impossible to directly observe but can be detected due to their gravitational effects. 'Rubin has enormous potential to help us learn what dark energy really is and how the universe's expansion is accelerating here, too,' Roodman said. 'Rubin's unique ability to see billions of galaxies and to image them repeatedly over 10 years will literally enable us to see the universe in a new way.'
