Table of Contents
NASA’s James Webb Space Telescope (JWST) has discovered a distant galaxy called “Firefly Sparkle.
Key Findings of James Webb Space Telescope (JWST)
Rate of Expansion: Data from the Webb telescope indicates that the universe’s expansion rate is approximately 8% faster than what is predicted based on current astrophysical models. This phenomenon is known as the Hubble Tension.
Hubble’s Law |
It is also known as the Hubble Constant, it says that the universe is expanding at a rate of 67-68 kilometers per second per megaparsec (a megaparsec is 3.26 million light-years). |
- Validation of Hubble’s Findings: The findings corroborate earlier measurements obtained from the Hubble Space Telescope, suggesting that the discrepancies are not due to instrument errors in Hubble.
Understanding Dark Matter and Dark Energy
- Dark Matter: Comprising about 27% of the universe, dark matter is an invisible form of matter inferred from its gravitational effects on visible matter.
- Dark Energy: Believed to constitute approximately 69% of the universe, dark energy is a hypothesized form of energy that drives the accelerated expansion of the universe.
Key Features of Firefly Sparkle
- Formation:
- The galaxy was formed 100–400 million years after the Big Bang.
- Its current observed state shows it as an infant galaxy, still in the process of assembling.
- Size and Structure:
- Mass: About 10 million stars, equivalent to the size of the Sun.
- Neighboring Galaxies: Two smaller neighboring galaxies named Firefly-Best Friend and Firefly-New Best Friend.
- Comparison with the Milky Way: At this stage, Firefly Sparkle is 10,000 times less massive than the present-day Milky Way.
Significance of the Discovery
- Insights into Galactic Formation: Firefly Sparkle provides a direct look at how galaxies like the Milky Way might have looked like in their infancy. Its mass and structure align with theoretical models of early Milky Way-like galaxies.
- Understanding Evolution: Firefly Sparkle represents the early formation phase in the evolutionary process of galaxies.
Gravitational Lensing
- Gravitational lensing is a phenomenon that occurs when a massive celestial body bends and warps space, causing light to bend and magnify.
- This effect allows astronomers to observe objects that would otherwise be too faint or distant to detect.
- Einstein’s General Theory of Relativity describes gravity not as a force between masses, but as the curvature of spacetime caused by mass and energy.
- Gravitational Lenses: The massive objects causing the bending of light are referred to as gravitational lenses. These can be individual stars, galaxies or clusters of galaxies.
- Without this effect, even the advanced JWST would not have been able to observe Firefly Sparkle due to its small size and distance.