Moon formation
A giant impact is the leading explanation for the Moon’s origin. Its exact sequence must account for the Moon’s composition, orbit and relationship to Earth.
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A giant impact is the leading explanation for the Moon’s origin. Its exact sequence must account for the Moon’s composition, orbit and relationship to Earth.
Ancient Martian rocks and landforms record liquid water under a fainter Sun. What climate sustained it, and how persistent were those wet conditions?
Uranus does release heat from its interior, despite older claims that it does not. How does its interior lose heat and produce the seasonal energy budget we observe?
A cooling liquid can become enormously slower without developing a crystal’s obvious order. What microscopic change explains its transition into a glass?
Old, metal-poor stars contain less lithium than standard early-universe calculations predict. Did the stars destroy it, or is something missing from the calculation or inference?
The collapse of a massive star can launch an explosion. Which stars explode, and can models predict the explosion and remnant from the star’s pre-collapse structure?
Starlight passing through interstellar gas picks up many absorption bands. Some have known molecular carriers, but most still lack a secure identification.
Planetary systems start with small solid grains. How do these become gravitationally bound bodies before collisions or inward drift remove them?
Earth’s moving plates are well established today. How and when did its early surface develop the connected system of recycling and motion we recognize as plate tectonics?
Two enormous regions near the bottom of Earth’s mantle slow seismic waves. What mixtures of heat and material create them, and how have they changed through time?
Airborne particles change how clouds form and reflect sunlight. How much cooling do those changes produce, across different clouds and weather conditions?
Neutrinos have three mass states. Which is heavier: the close pair or the third state?
Do neutrinos and antineutrinos change flavour differently in a way that violates charge–parity symmetry?
Proton-counting beam measurements and stored-neutron measurements give incompatible neutron lifetimes.
Does hot, baryon-rich nuclear matter have a critical endpoint where the character of its phase transition changes?
How does pressure depend on density inside a cold neutron star?
Which events supplied the rapid neutron-capture elements found throughout our Galaxy?
Which white-dwarf systems produce the different Type Ia supernovae?
What initial black holes grew into the massive objects seen in the early Universe?
Where did the seed magnetic fields amplified into cosmic magnetism come from?
How many ionizing photons escaped early galaxies and reached intergalactic hydrogen?
Where and how does the Sun regenerate the magnetic field underlying its activity cycle?
Which populations produce the diffuse high-energy neutrino flux measured by IceCube?
What microscopic interaction produces superconducting electron pairs across the cuprate phase diagram?