Monica Tavarez Frias -- Saint Patrick School of Santo Domingo, Dominican Republic
Introduction
What if the key to time travel isn’t hidden within the depths of...
Martina Guja Zagonel – Liceo Scientifico Bonaventura Cavalieri, Verbania, Italy
Introduction
With recent advancements and ongoing progress in Artificial Intelligence (AI), it's conceivable that in the...
Sebastian Sousa -- St. Patrick’s School of Santo Domingo, Dominican Republic
Introduction
Have you ever experienced an eerie coincidence? Thinking of someone just as they call...
Milena Niemczyk -- 1st Nicolaus Copernicus Secondary School, Bielsko-Biata, Poland
Introduction
Our eyes have always been directed towards the night sky. The inventions of the telescope and...
Marcus Mount -- Deer Valley High School, Antioch, CA, USA
When we think about it, space exploration is arguably humanity’s most exciting and monumental work. We...
Moneth Claire Corpuz -- Deer Valley High School, Antioch, CA, USA
“The sky is fake.”
Meina recalled the words of a delusional passerby near the Academy....
We investigate star formation in the Sc(s) II-III galaxy M33 by analyzing eight prominent HII regions using multi-wavelength data from the Spitzer Space Telescope and optical imagery. Results indicate that dust emission is a compact tracer of high-mass star formation, while PAH and H-alpha emissions decline more slowly with galactocentric radius.
Just like the dust that stubbornly besmirches your computer monitor, bookcase, and ancestral credenza, cosmic dust is now recognized to have a multiplicity of origins. For decades, astronomers thought that aging red giant stars produced most of the dust responsible for obscuring and reddening our views of nebulae and more distant stars ...
