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New Planets and Exoplanets Discovered by NASA

NASA has announced the discovery of Jupiter’s moon Jupiter II, the fourth planet that the Jovian system has found so far. It was the result of a global partnership between citizen scientists and professional astronomers. According to Paul Dalba, an astronomer at the University of California, Riverside, the signature for Jupiter’s moon was hidden in data from NASA’s Transiting Exoplanet Survey Satellite (TESS), which monitors the brightness of nearby stars. Changes in brightness indicate the presence of planets.

TIC 172900988 b

TIC 172900988 b is a planetary object that orbits a star called TIC. It is a relatively dense gas giant, with a mass of 2.84 MJ and radius of 0.9876 RJ. The star’s distance from Earth is approximately 2,405 light-years, or about 11.5 billion kilometers. It is the only planet that has two primary stars, both solar-mass G-type yellow dwarfs. It may have several large moons that are partly sheltered by Jupiter’s magnetic field.

In a bid to find out more about planetary systems, NASA’s Transiting Exoplanet Survey Satellite (TESS) has detected a circumbinary planet that orbits two stars. During its transit of the star, TIC 172900988 b appeared to make two dips in five days. As a result, this planetary system is actually a circumbinary binary. It is similar in size to Jupiter, but its orbit is longer than its parent star.

TOI 1338 b

Scientists have recently discovered a brand new exoplanet orbiting an F-type star, which is about 1,300 light years away. The planet is a gas world similar to Tatooine from Star Wars, and it is referred to as TOI 1338 b. Scientists have observed that the planet is 6.9 times larger than Earth and orbits two stars every 95 days. The astronomers studying the new planet used NASA’s TESS spacecraft to observe variations in the brightness of stars. The TESS satellite detects these variations and measures their distance from the stars.

Among the satellites that NASA has launched recently is TESS, a spacecraft that has been designed to search for bright, nearby worlds. This mission measures changes in the brightness of stars to detect the existence of habitable planets. TESS was used to discover TOI 1338 b, which orbits a cool, M dwarf star about 40 percent the mass of the Sun and about half the size of Earth.

A high school student from New York named Wolf Cukier was the first to discover the planet. In his internship at NASA’s Goddard Space Flight Center, Cukier was responsible for analyzing data collected by TESS, a spacecraft used to search for planets orbiting two stars. On the third day of his internship, Cukier found a blip in the data collected from one of the planet systems. The discovery of TOI-1338 b was announced at the 235th American Astronomical Society meeting.

The new discovery of a planet orbiting a star in the constellation Pictor has captivated the public. The TESS spacecraft, launched in 2018, was able to detect two planets instead of one. The planets orbit their star in a circumbinary system, which means that they orbit their star in two different directions. The Earth’s orbit is approximately six times that of TOI 1338 b, and each planet orbits its star twice a day.


NASA has found a brand-new planet outside our solar system. Kepler-1649c is an Earth-size exoplanet orbiting its star in a habitable zone, where rocky planets can support liquid water. It was misidentified by the telescope’s computer algorithm, but astronomers studying the data have recognized it as a world most like Earth. The discovery makes us wonder: is life really possible on other worlds?

In the Kepler-1649c discovery, researchers uncovered a rocky planet that orbits a red dwarf star. While it’s unlikely to support life on Earth, this type of world has a high probability of being habitable. As such, it is of particular interest to astronomers searching for potentially habitable worlds. However, there is still much to learn about Kepler-1649c.

Scientists using Kepler to find exoplanets use an algorithm called Robovetter to classify the data. This algorithm has been successful in finding more than 2,000 confirmed exoplanets and 2,500 promising candidates. The method works by detecting periodic dips in starlight caused by a planet’s passing in front of its host star. But this technique is not perfect, and many false positives may be due to other cosmic beings or variations in a star’s brightness.

While rocky planets are more likely to support life, exoplanets do not necessarily support life. Scientists are also unsure whether life exists on such worlds. In the meantime, researchers are exploring the possibility of life on the new planet. With the discovery of Kepler-1649c, scientists are now asking: “Can life exist on this new planet?”


A NASA new planet candidate named Kepler-854b is a gas giant exoplanet that orbits its host star in a 2.1-day orbit. It is approximately two times the mass of Jupiter and orbits at a distance of 0.0334 AU from its host star. Its mass makes it a potential candidate for being a planet, but there are some caveats to its planetary status.

The first hurdle in the confirmation of Kepler-854b’s new status as a NASA new planet is the astronomical distance. Because Kepler and Hubble measure stars’ sizes, the difference between their diameters was too large. When a star is over 4,000 light years away, its size is larger, and so the planet must be larger as well. Ultimately, Kepler and Hubble’s discoveries are both a good start for astronomical discovery.

A planet’s mass can be calculated using several methods. One of the most commonly used methods is a combination of mass and density. The mass of an exoplanet is only a rough estimate, but the astronomers say Kepler-854b is likely a super-Earth. Its rocky surface, thick clouds, and a high density make it appear like a world that might be habitable.

Other methods of confirming a new planet may include detecting a planet that is similar to Earth in mass. If Kepler-854b is indeed a planet, astronomers can further confirm the confirmation. Scientists say the new planet is close to Jupiter and will help explain the difference between a star and a planet. The discovery of Kepler-854b may also help us understand how planets form.


The team of astronomers at NASA has found a planet orbiting a star that is roughly two to three times the mass of Jupiter. The object is named Kepler-854b. The size of the planet is consistent with its host star’s changes in brightness. But is it really a planet? And why is it orbiting a star that is about three times the size of Jupiter?

According to NASA’s website, Kepler-699b is a gas giant that orbits a G-type star. Its mass is Unknown and it takes 27.8 days to complete its orbit. Kepler-699b is approximately 0.1711 AU from its star. It is the first planet discovered by the Kepler space telescope. Kepler-699b is a potential candidate for the naming of the next planet.

The Kepler Space Telescope has a large sample of data from astronomical observations. It has identified more than 2,000 exoplanet candidates, making it the most comprehensive collection of exoplanets announced at once. However, the new discovery contradicts evidence for the existence of four exoplanets previously confirmed by Kepler. These planets were discovered by NASA’s Kepler Space Telescope, which was responsible for most of the exoplanet discoveries.

Scientists have discovered 5,000 exoplanets with Kepler’s help. But three of them are not planets, and are actually stars. Researchers are still studying these new planets to determine their true size. Currently, NASA has confirmed a few of them as stars. Another eight exoplanet, Kepler-854b, is likely a star and will require more study.