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Which limit describes the brightness at which radiation pressure pushing matter outward balances gravity pulling it inward?

  1. A.Chandrasekhar limit
  2. B.Eddington limit
  3. C.Roche limit
  4. D.Schwarzschild radius

Correct answer

B. Eddington limit

Explanation

The correct answer is the Eddington limit. It is often used as a benchmark for how bright an accreting object can be, since beyond it the outward push of radiation would overwhelm the inward pull of gravity. Ultraluminous X-ray sources are puzzling precisely because they appear to shine more brightly than this simple balance predicts, and the new work concludes that ULX-8 is powered by a black hole accreting at rates exceeding this classical ceiling. Option A is wrong because the Chandrasekhar limit concerns the maximum mass of a stable white dwarf rather than a brightness ceiling. Option C is wrong because the Roche limit is the distance within which a body is torn apart by tidal forces. Option D is wrong because the Schwarzschild radius marks the event horizon of a non-rotating black hole, a size and not a luminosity.

Read the full article: IIA Team Traces Black Hole Behind Bright X-ray Source ULX-8

Q2.Science & TechnologyMedium

The research team that explained the behaviour of ULX-8 was drawn mainly from which institutes?

  1. A.Indian Institute of Astrophysics and Raman Research Institute
  2. B.Physical Research Laboratory and Space Applications Centre
  3. C.Tata Institute of Fundamental Research and Indian Institute of Science
  4. D.National Centre for Radio Astrophysics and Aryabhatta Research Institute
Show answer
Correct answer: A. Indian Institute of Astrophysics and Raman Research Institute

The paper was authored by Tarang Vashisht, a student at IISER Mohali, together with Aru Beri of the Indian Institute of Astrophysics and researchers from IUCAA and the Raman Research Institute.