There are documentaries about history, and then there are documentaries about the people who were quietly in the room when history happened.

STARMAN, the new film from Academy Award–nominated director Robert Stone, belongs firmly in the latter category. It chronicles the life of Gentry Lee—NASA scientist, mission architect, science communicator, and one of those rare figures whose career seems to map directly onto the modern Space Age.

If the Space Age began in 1957 with the launch of Sputnik, then Gentry Lee—born in 1942—has lived his entire adult life shaped by humanity’s reach beyond Earth. More than a witness to that history, Lee has been in the room for many of its defining moments.

As a senior scientist at NASA’s Jet Propulsion Laboratory, Lee served as Director of Science Analysis and Mission Planning for the Viking mission to Mars and the Galileo probe to Jupiter, missions that transformed our understanding of the solar system. Alongside this work, he collaborated with Carl Sagan on PBS’s landmark series COSMOS, narrated Discovery Channel’s ARE WE ALONE?, and co-authored four novels with legendary science fiction writer Arthur C. Clarke.

A Zelig-like figure at the crossroads of interplanetary science and science fiction, Gentry Lee has been everywhere—and worked with everyone—who helped define how we imagine space.

Now the subject of STARMAN, Lee guides us through a lifetime of curiosity, wonder, and exploration. The film is both entertaining and illuminating—and our conversation with him reflects that same spirit.

Scientists have long known that Earth’s core is mostly made of iron, but the density is not high enough for it to be pure iron, meaning lighter elements exist in the core, as well. In particular, it’s suspected to be a major reservoir of hydrogen. A new study, published in Nature Communications, supports this idea with results suggesting the core contains up to 45 oceans’ worth of hydrogen. These results also challenge the idea that most of Earth’s water was delivered by comets early on.

Because of the extreme conditions in Earth’s core and its distance from the surface, analyzing its composition presents difficulties. Additionally, many techniques are inadequate for resolving hydrogen because it is the lightest and smallest element. Earlier estimates relied on indirect methods, such as inferring hydrogen composition from lattice expansion in iron hydrides. These difficulties have led to highly uncertain estimates of hydrogen in the core, spanning four orders of magnitude.

The team involved in the new study took a different approach, using laser-heated diamond anvil cells to simulate high-pressure, high-temperature core conditions, up to 111 GPa and around 5,100 Kelvin. The team placed core-like iron samples and hydrous silicate glass, representing Earth’s early magma oceans, in the diamond anvil cells to induce melting, similar to conditions in the core.

Evidence from large-scale cosmic patterns suggests the universe may be fundamentally asymmetric.

Some stars appear to defy time itself. Nestled within ancient star clusters, they shine bluer and brighter than their neighbors, looking far younger than their true age. Known as blue straggler stars, these stellar oddities have puzzled astronomers for more than 70 years. Now, new results using the NASA/ESA Hubble Space Telescope are finally revealing how these “forever young” stars come to be and why they thrive in quieter cosmic neighborhoods.

Why blue stragglers puzzle astronomers Blue straggler stars stand out in old star clusters because they appear hotter, more massive and younger than stars that should all have formed billions of years ago. Their very existence contradicts standard theories of stellar aging, prompting decades of debate over whether they are created through violent stellar collisions or through more subtle interactions between pairs of stars.

A new study provides some of the clearest evidence yet that blue stragglers owe their youthful appearance not to collisions, but to life in close stellar partnerships, and to the environments that allow those partnerships to survive. The work is published in the journal Nature Communications.

There may be more to Musk’s decision to decide to build a city on the moon before building one on Mars than he’s telling us. Watch to find out.

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