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Solar Eclipse Resources

A spectacular eclipse will sweep across North America on April 8, 2024! Enjoy these free resources from the Astronomical Society of the Pacific!

Night-sky-network
Astronomical-society-of-the-pacific
Astronomical-society

NASA Reveals Plans To Broadcast Total Solar Eclipse – When To Watch

NASA Reveals Plans To Broadcast Total Solar Eclipse – When To Watch
forbes.com - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from forbes.com Daily Mail and Mail on Sunday newspapers.

Indiana
United-states
Niagara-falls
New-york
Russellville
Arkansas
Exploratorium
Illinois
Adirondack
Tupper-lake
Southern-illinois-university
Dallas

St. Lawrence University launches educational resources for Total Solar Eclipse 2024

CANTON — St. Lawrence University is celebrating its position within the path of totality with a new website dedicated to informing the public about the Total Solar Eclipse on April 8, 2024. The …

Connecticut
United-states
North-haven
China
Canton
Aileen-odonoghue
Tyler-karasinski
Astronomical-society-of-the-pacific
Lawrence-university
Total-solar-eclipse
Henry-priest-professor
Physics-aileeno-donoghue

'We are so excited': Eclipse gives Edinboro, other colleges a chance to teach

David Hurd’s excitement over what’s about to happen in the skies above him is obvious when he speaks. It even comes through in his voicemail these days. “We are so excited for April 8,” says the recorded message from Hurd, a geosciences professor and director of the planetarium at PennWest

Cincinnati
Ohio
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Meadville
Pennsylvania
Texas
Iowa
Grand-island
Nebraska
Thiel-college
Romania
Maine

A lanthanide-rich kilonova in the aftermath of a long gamma-ray burst

Observationally, kilonovae are astrophysical transients powered by the radioactive decay of nuclei heavier than iron, thought to be synthesized in the merger of two compact objects1–4. Over the first few days, the kilonova evolution is dominated by a large number of radioactive isotopes contributing to the heating rate2,5. On timescales of weeks to months, its behaviour is predicted to differ depending on the ejecta composition and the merger remnant6–8. Previous work has shown that the kilonova associated with gamma-ray burst 230307A is similar to kilonova AT2017gfo (ref. 9), and mid-infrared spectra revealed an emission line at 2.15 micrometres that was attributed to tellurium. Here we report a multi-wavelength analysis, including publicly available James Webb Space Telescope data9 and our own Hubble Space Telescope data, for the same gamma-ray burst. We model its evolution up to two months after the burst and show that, at these late times, the recession o

Chicago
Illinois
United-states
Sloan-digital-sky
Chicago-hubble-program
Astronomical-society-of-the-pacific
Astronomical-data-analysis-software
Mb-church
Carnegie-chicago-hubble
Los-alamos-supernova-light-curve-project
Conference-series

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