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Beiträge, die mit jwst getaggt sind


Wow wee, wow wow! JWST just keeps raising more questions than it's answering--& that's a good thing! JWST discovered that the toddler galaxy, GS-z13-1--which existed just 330 million years after the Big Bang--had ionized the ancestral neutral hydrogen that surrounded it allowing its light to transverse the universe & reach JWST. According to present hypothesis, that's incredibly early for a galaxy to have done that. https://www.esa.int/Science_Exploration/Space_Science/Webb/Webb_sees_galaxy_mysteriously_clearing_fog_of_early_Universe

#Astronomy #AstroPhysics #Cosmos #JWST #Science


Neue Daten vom #JWST stellen gängige Theorien auf den Kopf: Unerwartetes Rotationsmuster bei fernen Galaxien entdeckt. Astronomen rätseln über die Implikationen für unser Verständnis des Kosmos. https://winfuture.de/news,149573.html?utm_source=Mastodon&utm_medium=ManualStatus&utm_campaign=SocialMedia
#jwst


James-Webb-Teleskop könnte in nur 13 Stunden Beobachtungszeit Methylhalogenide auf Exoplaneten nachweisen. Ein Durchbruch für die Suche nach außerirdischem Leben? #JWST https://winfuture.de/news,149544.html?utm_source=Mastodon&utm_medium=ManualStatus&utm_campaign=SocialMedia
#jwst


Das #JWST hat beeindruckende Bilder des entstehenden Sternsystems Lynds 483 geliefert. Die Aufnahmen zeigen zwei junge Protosterne im Zentrum einer Gas- und Staubscheibe, umgeben von faszinierenden Strukturen. https://winfuture.de/news,149420.html?utm_source=Mastodon&utm_medium=ManualStatus&utm_campaign=SocialMedia
#jwst


Hot new #JWST image just dropped. (Literally hot; the temperature inside this object can reach upward of 25,000 degrees.)

Meet the planetary #nebula NGC 1514, aka the "Crystal Ball Nebula". It's about 1500 light years away from Earth in the direction of the constellation Taurus.

Planetary nebulae occur toward the end of the lives of #stars that have about the mass of the Sun. They shed their outer layers into space, leaving behind an Earth-sized star called a white dwarf. Its temperature can be up to about 100,000 degrees, so it emits a lot of ultraviolet and X-ray light. That light energizes the gas ejected during the earlier phase, lighting it up like a neon sign. (NGC 1514's white dwarf is the bright star at the center with the spikes, which are an artifact of the telescope's optics.)

This image is a composite of individual frames made through three colored filters by the Webb telescope's Mid-Infrared Instrument (MIRI). The image shows two concentric shells of material whose bright edges appear as circles. It's actually an hourglass-shaped structure seen an angle inclined to our line of sight toward NGC 1514.

A newly published study finds that these rings are different than the reddish material inside them. The light they emit comes from very tiny grains of carbon-rich material given off by the progenitor star very late in its life.

But why the ring shapes? It turns out that the progenitor star was actually two, only one of which endured this phase of high mass loss. Energetic "winds" given off by the stellar pair shaped the carbon grains as they were pushed away from the system.

(Processing of this image was done by Judy Schmidt: https://www.flickr.com/photos/geckzilla/54206737999)

#Astronomy
A colorful planetary nebula appears on a dark background. The nebula is a range of colors from red to pink to orange to white and consists of an inner reddish region surrounded by two diffuse gray/white rings tilted at 45 degrees toward the lower right. A bright star appears in the center with six short diffraction spikes. Faint stars and galaxies are scattered across the background.