JWST’s images improve on Hubble’s and narrow down the potential size of the star. The star appears as a point source of light suggesting it cannot be greater than 4000 astronomical units across. “These new observations strengthen the conclusion that Earendel is best explained by an individual star or multiple star system,” say Brian Welch at Johns Hopkins University in Baltimore and colleagues who have analyzed the images.
The team say that the photometry suggests Earendel has a surface temperature of between 13000 and 16000 Kelvin. This in turn suggests the star is a giant hydrogen-burning B-type star with a mass somewhere between 20 and 200 times that of the sun.
Is Earendel a binary star?
However, the team also say that Earendel could be a binary system and that various combinations of stars could better fit the observed data. Indeed, the best fit is a combination of a luminous cool star and a hot companion.
For the moment, the data does not allow the team to solve this problem. However, JWST is due to observe Earendel again later this year when more data could help to constrain the nature of this star or star system. It will also provide astronomers with more data about one the universe’s earliest stars.
That’s interesting work that shows off the extraordinary light gathering power of the JWST and its older relative Hubble, and how this instrument is already changing the way we see the universe.
Ref: JWST Imaging of Earendel, the Extremely Magnified Star at Redshift z=6.2: [*arxiv.org/abs/2208.09007