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An Afternoon of Family Science and Rocket Exploration in Alaska
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An Afternoon of Family Science and Rocket Exploration in AlaskaOn Tuesday, January 28th, Fairbanks BEST Homeschool joined the Geophysical Institute for an afternoon of rocket exploration, hands-on activities, and stargazing inside a planetarium. This event was free and open to the public. Despite their frigid winter weather, 200 attendees were curious about the scientific endeavors of Alaska-based researchers alongside cutting-edge investigations conducted by NASA rocket scientists.
Families and friends in attendance learned about two NASA rocket missions that would study the flickering and vanishing auroras: Ground Imaging to Rocket investigation of Auroral Fast Features (GIRAFF) and Black and Diffuse Aurora Science Surveyor (BaDASS). Visitors had an opportunity to sign up for text notifications related to the launch window. The planetarium presentations touch on Heliophysics Big Ideas that align with the three questions that drive NASA’s heliophysics research:
- What are the impacts of the changing sun on humanity?
- How do Earth, the solar system, and the heliosphere respond to changes on the sun?
- What causes the sun to vary?
The event also offered sun-related hands-on activities provided by the University of Alaska Museum of the North.
This event was offered to the community in association with the Science For Alaska Lecture Series and the 2025 NASA Sounding Rocket campaign. Every attendee left with something inspiring to think about. Parents and educators interested in learning more about auroras and do participatory science may check out NASA’s Aurorasaurus citizen science project.
The Geophysical Institute at the University of Alaska Fairbanks is a Co-Investigating team for the NASA Heliophysics Education Activation Team (NASA HEAT), which is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
Aurora Educational Resource List by Aurorasaurus
Families constructed and decorated their paper rockets.Katelin Avery It was so much fun! We are receiving rave reviews from our families and the surrounding community. THANK YOU AGAIN FOR COLLABORATING WITH US!Fairbanks BEST Homeschool
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A Stellar Bouquet
This image, released on Feb. 12, 2025, is the deepest X-ray image ever made of the spectacular star forming region called 30 Doradus. By combining X-ray data from NASA’s Chandra X-ray Observatory (blue and green) with optical data from NASA’s Hubble Space Telescope (yellow) and radio data from the Atacama Large Millimeter/submillimeter Array (orange), this stellar arrangement comes alive.
Otherwise known as the Tarantula Nebula, 30 Dor is located about 160,000 light-years away in a small neighboring galaxy to the Milky Way known as the Large Magellanic Cloud. Because it one of the brightest and populated star-forming regions to Earth, 30 Dor is a frequent target for scientists trying to learn more about how stars are born.
Learn more about this new image and what it reveals.
Image credit: X-ray: NASA/CXC/Penn State Univ./L. Townsley et al.; Infrared: NASA/JPL-CalTech/SST; Optical: NASA/STScI/HST; Radio: ESO/NAOJ/NRAO/ALMA; Image Processing: NASA/CXC/SAO/J. Schmidt, N. Wolk, K. Arcand
Hubble Captures a Cosmic Cloudscape
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Hubble Captures a Cosmic Cloudscape This NASA/ESA Hubble Space Telescope reveals clouds of gas and dust near the Tarantula Nebula, located in the Large Magellanic Cloud about 160,000 light-years away.ESA/Hubble & NASA, C. Murray Download this imageThe universe is a dusty place, as this NASA/ESA Hubble Space Telescope image featuring swirling clouds of gas and dust near the Tarantula Nebula reveals. Located in the Large Magellanic Cloud about 160,000 light-years away in the constellations Dorado and Mensa, the Tarantula Nebula is the most productive star-forming region in the nearby universe, home to the most massive stars known.
The nebula’s colorful gas clouds hold wispy tendrils and dark clumps of dust. This dust is different from ordinary household dust, which may include of bits of soil, skin cells, hair, and even plastic. Cosmic dust is often comprised of carbon or of molecules called silicates, which contain silicon and oxygen. The data in this image was part of an observing program that aims to characterize the properties of cosmic dust in the Large Magellanic Cloud and other nearby galaxies.
Dust plays several important roles in the universe. Even though individual dust grains are incredibly tiny, far smaller than the width of a single human hair, dust grains in disks around young stars clump together to form larger grains and eventually planets. Dust also helps cool clouds of gas so that they can condense into new stars. Dust even plays a role in making new molecules in interstellar space, providing a venue for individual atoms to find each other and bond together in the vastness of space.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Explore More Caldwell 103 / Tarantula Nebula / 30 Doradus Hubble Studies the Tarantula Nebula’s Outskirts Hubble’s New View of the Tarantula Nebula Hubble’s Bubbles in the Tarantula Nebula Hubble Probes Interior of Tarantula NebulaMedia Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Exploring the Birth of Stars
Hubble’s Night Sky Challenge
Hubble Focus: The Lives of StarsThis e-book highlights the mission’s recent discoveries and observations related to the birth, evolution, and death of stars.
