✨Aerin✨

I love waterfalls the are created and changed and often start through tectonic plate movements it is almost as thought mother herself is crying telling us to stop harming her and to stop altering her body and soul

The Running Chicken Nebula comprises several clouds, all of which we can see in this vast image from the VLT Survey Telescope (VST), hosted at ESO’s Paranal site. This 1.5-billion pixel image spans an area in the sky of about 25 full Moons. The clouds shown in wispy pink plumes are full of gas and dust, illuminated by the young and hot stars within them.

Today, we revealed the four astronauts who will fly around the Moon during the Artemis II mission, scheduled to launch in 2024. Get to know them:

Christina Koch

Meet the first member of our Artemis II crew: mission specialist Christina Koch. Koch visited the International Space Station in 2019, where she participated in the first all-woman spacewalk with Jessica Meir. She began her NASA career as an electrical engineer at Goddard Space Flight Center.

Jeremy Hansen

Representing the Canadian Space Agency is Jeremy Hansen from London, Ontario. Col. Hansen was a fighter pilot with Canadian Armed Forces before joining the Canadian Space Agency, and currently works with NASA on astronaut training and mission operations. This will be Col. Hansen’s first mission in space.

Victor Glover

Victor Glover is our Artemis II pilot. Glover is part of our 2013 class of NASA astronauts and was the pilot for NASA’s SpaceX Crew-1 mission. He’s logged 3,000 flight hours in more than 40 different aircraft.

Reid Wiseman

...and rounding out our Artemis II crew: mission commander Reid Wiseman. Wiseman lived and worked aboard the International Space Station as a flight engineer in 2014. He also commanded the undersea research mission NEEMO21, and most recently served as Chief of the NASA astronauts.

Carrier

*a little bit later*

This rare sight is a super-bright, massive Wolf-Rayet star. Calling forth the ephemeral nature of cherry blossoms, the Wolf-Rayet phase is a fleeting stage that only some stars go through soon before they explode.

The star, WR 124, is 15,000 light-years away in the constellation Sagittarius. It is 30 times the mass of the Sun and has shed 10 Suns worth of material – so far. As the ejected gas moves away from the star and cools, cosmic dust forms and glows in the infrared light detectable by NASA's James Webb Space Telescope.

The origin of cosmic dust that can survive a supernova blast is of great interest to astronomers for multiple reasons. Dust shelters forming stars, gathers together to help form planets, and serves as a platform for molecules to form and clump together, including the building blocks of life on Earth.

Stars like WR 124 also help astronomers understand the early history of the universe. Similar dying stars first seeded the young universe with heavy elements forged in their cores – elements that are now common in the current era, including on Earth.

The James Webb Space Telescope opens up new possibilities for studying details in cosmic dust, which is best observed in infrared wavelengths of light. Webb’s Near-Infrared Camera balances the brightness of WR 124’s stellar core and the knotty details in the fainter surrounding gas. The telescope’s Mid-Infrared Instrument reveals the clumpy structure of the gas and dust nebula of the ejected material now surrounding the star.

Omg they’re so cute I can’t 😭💗