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Lap1 B

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JWST uncovers the universe’s most primitive galaxy, LAP1-B
science1 month ago

JWST uncovers the universe’s most primitive galaxy, LAP1-B

The James Webb Space Telescope, aided by gravitational lensing from a foreground galaxy cluster, studied LAP1-B, a tiny galaxy formed about 800 million years after the Big Bang. Spectroscopy shows it has an exceptionally low oxygen abundance (about 1/240 of the Sun) and an elevated carbon-to-oxygen ratio, marking it as one of the most chemically primitive galaxies observed to date. The light was magnified roughly 100× by the MACS J0416 cluster, enabling insights into the early stages of galaxy formation and deeper connections to the Milky Way’s ancient fossil dwarf galaxies.

Webb Telescope Spots One of the Earliest Galaxies, Tracing the First Stars
astronomy1 month ago

Webb Telescope Spots One of the Earliest Galaxies, Tracing the First Stars

Using the James Webb Space Telescope, astronomers captured LAP1-B, one of the universe’s earliest and faint galaxies, dating to about 13 billion years ago (roughly 800 million years after the Big Bang). Gravitational lensing by a foreground cluster amplified its light ~100x, enabling spectroscopy that reveals extremely low metal content and signatures of Population III stars, including a high carbon-to-oxygen ratio. The data also suggest the galaxy sits in a massive dark matter halo, offering critical clues about how the first galaxies formed and evolved in the early cosmos (Nature).

JWST Finds the Most Metal-Poor Galaxy Yet, a Fossil from Cosmic Dawn
science1 month ago

JWST Finds the Most Metal-Poor Galaxy Yet, a Fossil from Cosmic Dawn

James Webb Space Telescope spectroscopy of LAP1-B, a strongly lensed galaxy at zspec ≈ 6.63, reveals an ultra-faint, chemically primitive star-forming system with gas-phase oxygen abundance of ~4×10−3 Z☉—the lowest yet for a high-redshift galaxy. It hosts a hard ionizing radiation field inconsistent with enriched populations, shows an elevated C/O ratio suggesting metal-free/poor stellar origins, and has a stellar mass <3,300 M⊙ while its dynamical mass exceeds baryons, implying a dominant dark-matter halo. LAP1-B is a direct high-redshift progenitor of local ultra-faint dwarfs, providing a rare window into early galaxy formation.