A peculiar and exceptionally hot celestial body, known as WD0032-317B, is setting new records and challenging astronomers' understanding of the line between stars and planets. As per Live Science, this object is categorized as a brown dwarf and resembles a bright, gaseous "protostar," which shares a comparable atmospheric composition to Jupiter but exceeds its size by 13 to 80 times.
With such mass, these entities initiate the fusion of hydrogen isotopes in their cores, yet they lack the necessary magnitude to sustain the full-fledged stellar fusion exhibited by stars like our sun, akin to smoldering charcoal rather than a fully ignited wood-fired oven.
Brown Dwarf Sheds Light on What Could Happen to Gas Giants Orbiting Massive Stars
The WD0032-317B exhibits an extraordinary temperature exceeding 8,000 Kelvin, significantly hotter than the surface of the Sun. As per Science Alert, this makes WD0032-317B the hottest brown dwarf ever detected. While brown dwarfs are hotter than planets, they remain cooler than the coolest red dwarf stars and cannot achieve the temperatures of our Sun through internal fusion processes.
The international research team, led by astrophysicist Na'ama Hallakoun from the Weizmann Institute of Science in Israel, named the object WD0032-317B. Their study, titled "An Irradiated-Jupiter Analogue Hotter Than the Sun" available in the preprint server arXiv and accepted into Nature Astronomy, sheds light on the behavior of gas giants similar to Jupiter that orbit extremely hot and massive stars.
Studying these exoplanets is challenging due to the stars' activity and rotation rates, which can obscure the signals from the orbiting planets. Close proximity to a bright star subjects planets to intense ultraviolet radiation, leading to the evaporation and dissociation of their atmospheres.
KELT-9b, an exoplanet orbiting a blue supergiant star, is the only other known planet with temperatures high enough for thermal dissociation. Its day side reaches temperatures exceeding 4,600 Kelvin.
To investigate such extreme environments, scientists propose studying brown dwarfs in binary systems with white dwarf stars. White dwarfs, which are much smaller and dimmer than blue supergiants, make it easier to isolate the signals from any companion objects heated to extreme temperatures.
Exploring WD0032-317B and similar objects provides valuable insights into the dynamics and characteristics of celestial bodies in extreme environments, contributing to our understanding of the boundaries between planets and stars and the effects of close stellar proximity on exoplanetary atmospheres.
Discovery of the Peculiar Brown Dwarf
In early 2000, a research team analyzing data from the European Southern Observatory's Very Large Telescope discovered an intriguing celestial object, WD0032-317.
According to Phys.org, it was initially believed to be a companion star, but further investigation revealed that it is a brown dwarf. With a mass estimated to be between 75 and 88 times that of Jupiter, WD0032-317B orbits its star at a remarkably fast rate of only 2.3 hours.
The researchers also observed that the brown dwarf is tidally locked, resulting in extreme temperature differences between its sides. The hot side experiences temperatures ranging from approximately 7,250 to 9,800 Kelvin, while the cooler side ranges from approximately 1,300 to 3,000 Kelvin.
Remarkably, the temperatures on the hot side exceed those of any other known giant planet by approximately 5,100 Kelvin. This makes WD0032-317B the hottest recorded brown dwarf and surpasses the temperatures of all known planets.
RELATED ARTICLE: NASA James Webb Space Telescope Finds Giant Brown Dwarf 31x Larger Than Jupiter [LOOK]
Check out more news and information on Space in Science Times.
