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Mira Stars Aid in Most Precise Measurement of Universe’s Expansion Rate

IUCAA Scientists Harness Variable Giants as Standard Candles in the Extragalactic Distance Ladder

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Mira Stars Aid in Most Precise Measurement of Universe’s Expansion Rate

Introduction:

  • Scientists at the Inter-University Centre for Astronomy and Astrophysics (IUCAA), Pune, have recently achieved the most precise determination of the expansion rate of the universe using Mira variable stars.
  • This work enhances our understanding of the Hubble Constant, a fundamental parameter in cosmology.

About Mira Stars:

  • Mira, also known as Omicron Ceti, is a red giant star located about 300 light-years away in the constellation Cetus.
  • The name Mira means “the wonderful” in Latin.
  • It became the first variable star ever discovered (observed in 1596 by David Fabricius, studied further in the 17th century).
  • Mira stars are typically 200–400 times larger than the Sun but much cooler, with a surface temperature of about 3,000 Kelvin (Sun: ~6,000 K).

Characteristics of Mira Variables:

  • They are pulsating red giants in the late stages of stellar evolution.
  • Brightness variation cycle: 100 to 1,000 days.
  • They can change brightness by a factor of 10 to 1,000 times during each pulsation cycle.
  • Mass loss through stellar winds: up to 10⁻⁷ solar masses per year, enriching the interstellar medium.

Astronomical Importance:

  • Mira variables follow a clear Period–Luminosity (P–L) relationship, similar to Cepheid variables but cooler and older.
  • This makes them reliable standard candles for measuring cosmic distances up to several million light-years.
  • Standard candles are crucial to build the Extragalactic Distance Ladder, used to estimate distances beyond the Milky Way.

Recent Development by IUCAA:

  • IUCAA scientists calibrated Mira stars with unprecedented accuracy using infrared observations, where they shine brightest.
  • Their study allowed a refined measurement of the Hubble Constant (H₀), which describes how fast the universe is expanding.
  • This is important in the context of the ongoing “Hubble Tension” – a discrepancy between H₀ values derived from the early universe (Cosmic Microwave Background, ~67 km/s/Mpc) and the late universe (Cepheids/Supernovae, ~73 km/s/Mpc).
  • Mira stars provide an independent method to test and potentially resolve this tension.

Global Relevance:

  • Adds another rung to the cosmic distance measurement toolkit.
  • Helps refine models of dark energy, galaxy evolution, and the fate of the universe.
  • Complements other standard candles like Cepheids and Type Supernovae.

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