Its updated planetary parameters from Chachan et al. However, perhaps the more interesting news this week is about the new parameter sets that include more accurate mass measurements for two known planets: Kepler-167 e and eps Eri b.Kepler-167 e is the only known transiting Jupiter analog outside of 1 AU that also has inner rocky planets. We’ve added three new planets this week: TOI-1422 b, GJ 3512 c, and CoRoT-7 d. * TESS Project Candidates Yet To Be Confirmed refers to the number of TESS Project Candidates that have not yet been dispositioned as a Confirmed Planet or False Positive.Ĭlick here to see NASA’s interactive exoplanet website Exoplanet News: JThree Planets and New Masses for Two Planets * TESS Project Candidates refers to the total number of transit-like events that appear to be astrophysical in origin, including false positives as identified by the TESS Project. * Confirmed Planets Discovered by TESS refers to the number planets that have been published in the refereed astronomical literature. TESS Project Candidates Integrated into Archive ( 13:00:01)Ĭurrent date TESS Project Candidates at ExoFOP Kepler Project Candidates Yet To Be Confirmed et /ˈeksōˌplanət/, noun: a planet orbiting a star other than the Sun.MAG is the visual magnitude of the asteroid on the date of closest approach.Įx Notes: LD means “Lunar Distance.” 1 LD = 384,401 km, the distance between Earth and the Moon. Upcoming Earth-asteroid encounters: Asteroid Total Minor Planets discovered ( MPC): 1,217,569 ( +10,232 updated ).Potentially Hazardous Asteroids (PHAs): 2276 (+4 updated ).Near-Earth Objects (NEOs) discovered this month: 59, this year: 1441 (+28), all time: 29,253 (+28).On Twitter, Facebook, Google News, and Instagram. The glowing gas filaments across the image left, like supernova remnants in our own galaxy, testify to violent stellar explosions and indicate that short-lived massive stars have recently been present in the region.įollow HT Tech for the latest tech news and reviews, also keep up with us Stars in the large cluster are estimated to be 50 million years young, while stars in the compact cluster are younger still, with an age of about 4 million years.Ī mere 168,000 light-years distant, NGC 1850 is located near the outskirts of the Large Magellanic Cloud galaxy. Moreover, NGC 1850 is also a double star cluster, with a second, compact cluster of stars visible here just to the right of the large cluster's center. ![]() But NGC 1850's stars are all too young, making it a type of star cluster with no known counterpart in the Milky Way. This is surprising because, at first glance, this featured image by the Hubble Space Telescope suggests that star cluster NGC 1850's size and shape are reminiscent of the many ancient globular star clusters which roam our own Milky Way Galaxy's halo. There is nothing like this ball of stars in our Milky Way Galaxy. This proves yet again that the space telescope might be old, but it is still capable of capturing breathtaking images of celestial objects located even millions of light-years away. The picture was captured by the Hubble Space Telescope, which is run by NASA and ESA in collaboration.
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