Whatsupinspace

NASA is boosting cyber to space using a technology called Disruption Tolerant Networking. The technology will help overcome several space communications challenges, benefiting missions in Earth orbit and those farther out in the solar system. Disruption Tolerant Networking also has future Earth-based applications. Learn more about Disruption Tolerant Networking: www.nasa.gov/content/dtn

Is there oxygen on Mars? Technically yes, but it’s nothing like the amount we have on Earth. So breathing is out of the question. However, there IS a lot of carbon dioxide (CO2) on Mars. Now a new technology — MOXIE — has proven that we can convert Martian CO2 into oxygen for use by future explorers.

This video tours areas of Webb’s near-infrared light view of the Pillars of Creation. This area is brimming with gas and dust – which are essential ingredients for star formation. Glowing, bright red wavy lines appear at the edges of some pillars, revealing where stars are ejecting material as they form. The bright red orbs are newly formed stars that have burst into view. Distant galaxies typically make appearances in Webb’s images, but not this one. A translucent layer of gas and dust is drawn like a curtain, allowing the stars to take centerstage. Webb’s near-infrared image will help researchers update their models of star formation. Over time, we’ll learn how stars form and burst out of these dusty clouds over millions of years.

Water in space behaves… differently. Surface tension and capillary flow can be harnessed to move fluids in more efficient ways. What looks like fun could actually help us improve systems for moving fluids in microgravity, in things like fuel tanks for space travel.

While Apollo placed the first steps on the Moon, Artemis opens the door for humanity to sustainably work and live on another world for the first time. Using the lunar surface as a proving ground for living on Mars, this next chapter in exploration will forever establish our presence in the stars. ✨ We are returning to the Moon – to stay – and this is how we are going!