One of the greatest cosmic mysteries today concerns the expansion of the universe.
Two main methods each give low error answers, but are not compatible.
By tracing the evolution of an early relic signal, we measure an expansion of 67 km/s/mq.
By starting close and noticing the slack increasing with distance, we measure 73 km/s/m per square metre.
This discrepancy – the “Hubble tension” – is a recent cosmic mystery.
Many would expect a note error on the “distance ladder” side to be the culprit.
We begin by observing Cepheid variable stars within the Milky Way.
We infer their exact distances by parallax.
Then we measure Cepheids in well-measured nearby galaxies.
Finally, we measure Type Ia supernovae both inside and outside those galaxies, and relate these cosmic “degrees” together.
Could the error in Cepheids be biasing our measured expansion rate?
by Cepheids measured in nearby galaxiesJWST investigates this possibility.
galaxy watch NGC 4258JWST found no optical bias for Algivides.
Instead, it confirmed and reinforced previous Hubble Space Telescope findings.
Cepheids in NGC 5584which she also had A (2007 epoch) a Type Ia supernovaalso revealing no bias.
the Gloss relationship periodthe main calibration tool for Chronology, is now more accurate than ever.
Thanks to its superior accuracy, JWST has reduced any uncertainties down to their absolute smallest values.
Mostly Mute Monday tells an astronomical story with pictures and visuals and no more than 200 words.
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