RT @Wikisteff: This cool paper measured the rotation rates of young planemos (sub-brown dwarfs), and found they were largely set in late ac…
This cool paper measured the rotation rates of young planemos (sub-brown dwarfs), and found they were largely set in late accretion by disc interactions, possibly explaining why our planets mostly spin around a vertical axis. https://t.co/a5F127ocbx
...AND this other one packed with cool insights on the rotation evolution of planets and brown dwarfs by Bryan et al https://t.co/8trQs3ZLlk
#universe #space #nasa #physics Constraints on the spin evolution of young planetary-mass companions https://t.co/iSYyj1ddNX
#universe #space #nasa #physics Constraints on the spin evolution of young planetary-mass companions https://t.co/iSYyj1ddNX
RT @NatureAstronomy: Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Br…
#universe #space #nasa #physics Constraints on the spin evolution of young planetary-mass companions https://t.co/iSYyj1ddNX
Constraints on the Spin Evolution of Young Planetary-Mass Companions: https://t.co/6rsZac1D7M -> https://t.co/BEqtXZkdnt
RT @NatureAstronomy: Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Br…
RT @AstroPHYPapers: Constraints on the Spin Evolution of Young Planetary-Mass Companions. https://t.co/vhKO02DNro
Constraints on the Spin Evolution of Young Planetary-Mass Companions. https://t.co/vhKO02DNro
RT @NatureAstronomy: Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Br…
Constraints on the spin evolution of young planetary-mass companions https://t.co/uqUmHG9AYc via @NatureAstronomy https://t.co/248RXkiW3z
#DataScience #ai #bigdata Constraints on the spin evolution of young planetary-mass companions https://t.co/iSYyj1ddNX
RT @NatureAstronomy: Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Br…
RT @NatureAstronomy: Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Br…
Constraints on the spin evolution of young planetary-mass companions https://t.co/xdxphxHZrP https://t.co/NExSDXNmp0
Rotation rates of young planetary-mass objects are set late in the accretion stage and don’t evolve after ~100 Myr. Bryan et al.: https://t.co/nKRdsoqbLo https://t.co/VZe2YFAxHM