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|    ScienceDaily to All    |
|    Life after death: Astronomers find a pla    |
|    28 Jun 23 22:30:20    |
      MSGID: 1:317/3 649d08ee       PID: hpt/lnx 1.9.0-cur 2019-01-08       TID: hpt/lnx 1.9.0-cur 2019-01-08        Life after death: Astronomers find a planet that shouldn't exist                Date:        June 28, 2023        Source:        University of Hawaii at Manoa        Summary:        The star would have inflated up to 1.5 times the planet's orbital        distance -- engulfing the planet in the process -- before shrinking        to its current size at only one-tenth of that distance.                      Facebook Twitter Pinterest LinkedIN Email              ==========================================================================       FULL STORY       ==========================================================================       When our Sun reaches the end of its life, it will expand to 100 times its       current size, enveloping the Earth. Many planets in other solar systems       face a similar doom as their host stars grow old. But not all hope is       lost, as astronomers from the University of Hawaii Institute for Astronomy       (UH IfA) have made the remarkable discovery of a planet's survival after       what should have been certain demise at the hands of its sun.              The Jupiter-like planet 8 UMi b, officially named Halla, orbits the red       giant star Baekdu (8 UMi) at only half the distance separating the Earth       and the Sun.              Using two Maunakea Observatories on Hawaiii Island -- W. M. Keck       Observatory and Canada-France-Hawaii Telescope (CFHT) -- a team       of astronomers led by Marc Hon, a NASA Hubble Fellow at UH IfA, has       discovered that Halla persists despite the normally perilous evolution of       Baekdu. Using observations of Baekdu's stellar oscillations from NASA's       Transiting Exoplanet Survey Satellite (TESS), they found that the star       is burning helium in its core, signaling that it had already expanded       enormously into a red giant star once before.              The star would have inflated up to 1.5 times the planet's orbital       distance - - engulfing the planet in the process -- before shrinking to       its current size at only one-tenth of that distance.              The study is published in today's issue of the journal Nature.              "Planetary engulfment has catastrophic consequences for either the       planet or the star itself -- or both. The fact that Halla has managed       to persist in the immediate vicinity of a giant star that would have       otherwise engulfed it highlights the planet as an extraordinary survivor,"       said Hon, the lead author of the study.              Maunakea Observatories Confirm the Survivor The planet Halla was       discovered in 2015 by a team of astronomers from Korea using the radial       velocity method, which measures the periodic movement of a star due to       the gravitational tug of the orbiting planet. Following the discovery       that the star must at one time have been larger than the planet's orbit,       the IfA team conducted additional observations from 2021-2022 using Keck       Observatory's High-Resolution Echelle Spectrometer (HIRES) and CFHT's       ESPaDOnS instrument. These new data confirmed the planet's 93-day,       nearly circular orbit had remained stable for over a decade and that       the radial velocity changes must be due to a planet.              "Together, these observations confirmed the existence of the planet,       leaving us with the compelling question of how the planet actually       survived," said IfA astronomer Daniel Huber, second author of the       study. "The observations from multiple telescopes on Maunakea was       critical in this process." Escaping Engulfment At a distance of 0.46       astronomical units (AU, or the Earth-Sun distance) to its star, the       planet Halla resembles 'warm' or 'hot' Jupiter-like planets that are       thought to have started on larger orbits before migrating inward close to       their stars. However, in the face of a rapidly evolving host star, such       an origin becomes an extremely unlikely survival pathway for planet Halla.              Another theory for the planet's survival is that it never faced the       danger of engulfment. Similar to the famous planet Tatooine from Star       Wars, which orbits two suns, the team believes the host star Baekdu may       have originally been two stars. A merger of these two stars may have       prevented any one of them from expanding sufficiently large enough to       engulf the planet.              A third possibility is that Halla is a relative newborn -- that the       violent collision between the two stars produced a gas cloud from which       the planet formed. In other words, the planet Halla may be a recently-born       'second generation' planet.              "Most stars are in binary systems, but we don't yet fully grasp how       planets may form around them. Therefore, it's plausible that more       planets may actually exist around highly evolved stars thanks to binary       interactions," explained Hon.               * RELATED_TOPICS        o Space_&_Time        # Extrasolar_Planets # Stars # Astronomy # Jupiter #        Kuiper_Belt # Eris_(Xena) # Mars # Pluto        * RELATED_TERMS        o Venus o Eris_(dwarf_planet) o Precession o Uranus o Axial_tilt        o Moon o Neptune o Definition_of_planet              ==========================================================================       Story Source: Materials provided by University_of_Hawaii_at_Manoa. Note:       Content may be edited for style and length.                     ==========================================================================       Related Multimedia:        * Artist's_impression_of_the_planet's_survival       ==========================================================================       Journal Reference:        1. Marc Hon, Daniel Huber, Nicholas Z. Rui, Jim Fuller, Dimitri        Veras, James        S. Kuszlewicz, Oleg Kochukhov, Amalie Stokholm, Jakob Lysgaard        Ro/rsted, Mutlu Yıldız, Zeynep C,elik Orhan, Sibel O"rtel,        Chen Jiang, Daniel R. Hey, Howard Isaacson, Jingwen Zhang, Mathieu        Vrard, Keivan G.               Stassun, Benjamin J. Shappee, Jamie Tayar, Zachary R. Claytor,        Corey Beard, Timothy R. Bedding, Casey Brinkman, Tiago L. Campante,        William J.               Chaplin, Ashley Chontos, Steven Giacalone, Rae Holcomb, Andrew        W. Howard, Jack Lubin, Mason MacDougall, Benjamin T. Montet, Joseph        M. A. Murphy, Joel Ong, Daria Pidhorodetska, Alex S. Polanski,        Malena Rice, Dennis Stello, Dakotah Tyler, Judah Van Zandt,        Lauren M. Weiss. A close-in giant planet escapes engulfment by its        star. Nature, 2023; 618 (7967): 917 DOI: 10.1038/s41586-023-06029-0       ==========================================================================              Link to news story:       https://www.sciencedaily.com/releases/2023/06/230628130343.htm              --- up 1 year, 17 weeks, 2 days, 10 hours, 50 minutes        * Origin: -=> Castle Rock BBS <=- Now Husky HPT Powered! (1:317/3)       SEEN-BY: 15/0 106/201 114/705 123/120 153/7715 218/700 226/30 227/114       SEEN-BY: 229/110 112 113 307 317 400 426 428 470 664 700 291/111 292/854       SEEN-BY: 298/25 305/3 317/3 320/219 396/45 5075/35       PATH: 317/3 229/426           |
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