Astronomers working with TESS (Transiting Exoplanet Survey Satellite) have discovered a planet that’s been left out in the Sun too long. Or at least half of it has. The newly discovered planet is tidally locked to its star, and one side is completely molten.
Continue reading “Half of this Exoplanet is Covered in Lava”A Planetary System With Six Sub-Neptunes Locked in Perfect Resonance
A team of researchers led by University of Chicago astronomer Rafael Luque analyzed data acquired by both NASA’s Transiting Exoplanet Survey Satellite (TESS) and ESA’s CHaracterising ExOPlanet Satellite (Cheops) and found a unique planetary system. Orbiting a star cataloged as HD110067, this system contains six sub-Neptune planets. Incredibly, all six planets are orbiting in direct resonance with each other. The results of the work were published on November 29 in Nature.
Continue reading “A Planetary System With Six Sub-Neptunes Locked in Perfect Resonance”This Exoplanet is Probably a Solid Ball of Metal
We can’t understand nature without understanding its range. That’s apparent in exoplanet science and in our theories of planetary formation. Nature’s outliers and oddballs put pressure on our models and motivate scientists to dig deeper.
Continue reading “This Exoplanet is Probably a Solid Ball of Metal”TESS Finds a Planet That Takes 482 Days to Orbit, the Widest it’s Seen so Far
We’re rapidly learning that our Solar System, so familiar to us all, does not represent normal.
A couple of decades ago, we knew very little about other solar systems. Astronomers had discovered only a handful of exoplanets, especially around pulsars. But that all changed in the last few years.
Continue reading “TESS Finds a Planet That Takes 482 Days to Orbit, the Widest it’s Seen so Far”Astronomers Find an Earth-Sized World That May Be Carpeted in Volcanoes
Astronomers think they’ve found an extrasolar planet covered in volcanoes like Jupiter’s moon Io, but this world is about the same size as Earth. Designated LP 791-18 d, the planet is probably tidally locked around a small, red dwarf star about 90 light-years away in the constellation Crater. There are two other more massive planets in the system, and their tidal interactions could cause enough tidal flexing that it unleashes planet-wide volcanoes on LP 791-18 d.
Planet d is located within the habitable zone of the star, and with all the other conditions, astronomers think it might be temperate enough on the permanent night side of this world to allow water to exist.
Continue reading “Astronomers Find an Earth-Sized World That May Be Carpeted in Volcanoes”Two Super-Earths Found Orbiting a Red Dwarf Star at the Edge of the Habitable Zone
NASA’s Transiting Exoplanet Survey Satellite, or TESS, was designed to find other worlds. Following in the tradition of the Kepler spacecraft, TESS has a hundred thousand stars looking for small but regular dips in their brightness. These dips are typically caused by planets as they pass in front of the star. TESS has been quite effective, logging nearly 6,000 candidate exoplanets. Confirming or rejecting these candidates takes time, but it has led to some interesting discoveries.
Continue reading “Two Super-Earths Found Orbiting a Red Dwarf Star at the Edge of the Habitable Zone”TESS Reaches Fifth Anniversary of Extraordinary Mission, but its Work is Far from Over
NASA’s TESS (Transiting Exoplanet Survey Satellite) mission recently reached its fifth anniversary of service to humanity as it continues to tirelessly scan the heavens for worlds beyond. Dubbed as an all-sky mission, TESS was launched on April 18, 2018, aboard a SpaceX Falcon rocket. During its five years in space, TESS’s four 24 degrees by 24 degrees field-of-view CCD cameras have successfully mapped greater than 93% of the cosmos.
Continue reading “TESS Reaches Fifth Anniversary of Extraordinary Mission, but its Work is Far from Over”The Planet That Shouldn’t Exist
As of this writing, almost 5300 exoplanets spanning approximately 4000 planetary systems have been confirmed to exist in our universe. With each new exoplanet discovery, scientists continue to learn more about planetary formation and evolution that has already shaken our understanding of this process down to its very core. One such example is “Hot Jupiters”, which are Jupiter-sized exoplanets, or larger, that orbit closer to their parents stars than Mercury does to our own. This is in stark contrast to our own Solar System, which has rocky planets closer towards our Sun and the gas giant planets much farther out.
Continue reading “The Planet That Shouldn’t Exist”TESS has Found A Second Earth-Sized World in This System. Exoplanet Science is Maturing
For planet-hunters, finding an Earth-sized exoplanet must be special. NASA estimates there are about 100 billion planets in the Milky Way, but the large majority of the 5,000+ exoplanets we’ve found are extremely inhospitable. So finding one that’s similar to ours is kind of comforting.
In this case, it’s even more interesting because it’s the second Earth-sized planet orbiting the same star.
Continue reading “TESS has Found A Second Earth-Sized World in This System. Exoplanet Science is Maturing”Astronomers Directly Image Debris Disk and find a Jupiter-Sized Planet Orbiting a Sunlike Star
According to the most widely-accepted theory, planetary systems form from large clouds of dust and gas that form disks around young stars. Over time, these disks accrete to create planets of varying size, composition, and distance from their parent star. In the past few decades, observations in the mid- and far-infrared wavelengths have led to the discovery of debris disks around young stars (less than 100 million years old). This has allowed astronomers to study planetary systems in their early history, providing new insight into how systems form and evolve.
This includes the SpHere INfrared survey for Exoplanets (SHINE) consortium, an international team of astronomers dedicated to studying star systems in formation. Using the ESO’s Very Large Telescope (VLT), the SHINE collaboration recently directly imaged and characterized the debris disk of a nearby star (HD 114082) in visible and infrared wavelengths. Combined with data from NASA’s Transiting Exoplanet Space Satellite (TESS), they were able to detect a gas giant many times the size of Jupiter (a “Super-Jupiter”) embedded within the disk.
Continue reading “Astronomers Directly Image Debris Disk and find a Jupiter-Sized Planet Orbiting a Sunlike Star”