Description
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Source: Moneycontrol
Context
Scientists just discovered TOI-6894b, a huge planet circling a very small red dwarf star, challenging previous beliefs.
What is TOI-6894b?
TOI-6894b, a gas giant planet around the size of Saturn, has been discovered orbiting an abnormally small red dwarf star.
Features of the planet
- This unusual coupling contradicts existing theories, which state that tiny stars do not have enough material in their surrounding disks to generate such huge planets.
- The planet was discovered in the constellation Leo, approximately 241 light years away from Earth.
- TOI-6894b is approximately 1.07 times the diameter of Saturn, but weighs slightly more than half of it.
- This results in the planet having a relatively low density, akin to that of a beach ball. Despite its huge size, the planet circles very close to its home star, completing a full revolution in slightly under three Earth days.
- TOI-6894, the star it circles, is a red dwarf that is only about 21% the mass of the Sun and around 250 times fainter.
- In terms of physical dimensions, the star is only 2.5 times wider than the planet, an unusual size ratio in planetary systems.
Theories related to the discovery
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Challenges to Core Accretion Theory
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The core accretion model struggles to explain the formation of a giant planet like TOI-6894b around a low-mass star due to limited material in the disk.
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Implications for Exoplanet Science
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The discovery suggests that gas giants may be more common around small stars than previously believed, challenging existing models of planetary formation.
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Future Studies
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TOI-6894b is set for atmospheric observation by the James Webb Space Telescope (JWST), which may reveal detailed insights into its composition and origin.
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Source: Sciencedaily.com
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Practice Question:
Q. Consider the following statements about TOI-6894b:
- It is an exoplanet classified as an ultrahot Jupiter.
- It orbits a high-mass, Sun-like star located in the Andromeda Galaxy.
- The planet challenges the core accretion theory of planet formation.
- It is scheduled for atmospheric observation by the James Webb Space Telescope (JWST).
Which of the statements given above is/are correct?
Options:
(a) 1, 2 and 4 only (b) 1, 3 and 4 only (c) 2 and 3 only (d) 1 and 3 only
Correct Answer:
(b) 1, 3 and 4 only
Explanation:
- Statement 1 – Correct: TOI-6894b is classified as an ultrahot Jupiter, a type of gas giant with very high surface temperatures.
- Statement 2 – Incorrect: TOI-6894b orbits a low-mass star, not a high-mass Sun-like star, and is located within the Milky Way, not in the Andromeda Galaxy.
- Statement 3 – Correct: The discovery challenges the core accretion theory, which struggles to explain how such a planet forms around a low-mass star.
- Statement 4 – Correct: TOI-6894b is scheduled for atmospheric study by JWST, which could offer insights into its formation and composition.
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