A groundbreaking study suggests that our early Sun may have been encircled by massive rings of dust—structures that shaped the very layout of our Solar System and may have prevented Earth from becoming a super-Earth.
According to researchers, these dusty rings were created by pressure “bumps”—high-pressure zones caused as particles spiraled inward, heated up, and released gases through vaporization.
These zones formed sublimation lines, where materials like silicates, water ice, and carbon monoxide turned from solid to gas. As a result, dust got trapped instead of falling into the Sun, clumping into planetesimals—the seeds of planets.
Simulations showed that:
The inner ring gave rise to Mercury, Venus, Earth, and Mars
The middle ring helped birth the gas giants
The outer ring contributed to comets, asteroids, and Kuiper Belt objects
Interestingly, had the middle ring formed a bit later, more material could have gathered in the inner Solar System—potentially allowing super-Earths to form. Their absence is one of the mysteries that sets our planetary system apart from others across the galaxy.
RESEARCH PAPER
Andre Izidoro et al., Planetesimal rings as the cause of the Solar System’s planetary architecture, Nature Astronomy (2022)
According to researchers, these dusty rings were created by pressure “bumps”—high-pressure zones caused as particles spiraled inward, heated up, and released gases through vaporization.
These zones formed sublimation lines, where materials like silicates, water ice, and carbon monoxide turned from solid to gas. As a result, dust got trapped instead of falling into the Sun, clumping into planetesimals—the seeds of planets.
Simulations showed that:
The inner ring gave rise to Mercury, Venus, Earth, and Mars
The middle ring helped birth the gas giants
The outer ring contributed to comets, asteroids, and Kuiper Belt objects
Interestingly, had the middle ring formed a bit later, more material could have gathered in the inner Solar System—potentially allowing super-Earths to form. Their absence is one of the mysteries that sets our planetary system apart from others across the galaxy.
RESEARCH PAPER
Andre Izidoro et al., Planetesimal rings as the cause of the Solar System’s planetary architecture, Nature Astronomy (2022)
A groundbreaking study suggests that our early Sun may have been encircled by massive rings of dust—structures that shaped the very layout of our Solar System and may have prevented Earth from becoming a super-Earth.
According to researchers, these dusty rings were created by pressure “bumps”—high-pressure zones caused as particles spiraled inward, heated up, and released gases through vaporization.
These zones formed sublimation lines, where materials like silicates, water ice, and carbon monoxide turned from solid to gas. As a result, dust got trapped instead of falling into the Sun, clumping into planetesimals—the seeds of planets.
Simulations showed that:
The inner ring gave rise to Mercury, Venus, Earth, and Mars
The middle ring helped birth the gas giants
The outer ring contributed to comets, asteroids, and Kuiper Belt objects
Interestingly, had the middle ring formed a bit later, more material could have gathered in the inner Solar System—potentially allowing super-Earths to form. Their absence is one of the mysteries that sets our planetary system apart from others across the galaxy.
RESEARCH PAPER
Andre Izidoro et al., Planetesimal rings as the cause of the Solar System’s planetary architecture, Nature Astronomy (2022)


