4. Scientists have long debated the origins of the
solar system.
• In the 1600s and 1700s, many scientists
thought the sun formed first and produced
materials which later formed the planets.
6. The Protoplanet Theory
According to this theory, dense interstellar
cloud produces a cluster of stars
-small blobs spins randomly resulting to the
low rotation of stars that lead to the formation
of “planetary blobs”
The 'planetary blobs' split into planets and
satellites.
7. Planetesimal Hypothesis
According to this theory, tiny solid
particles or "planetesimals" in the
protoplanetary disk clumped together
through collisions and gravitational
attraction to form larger bodies, which
eventually became planets.
This process is often considered a key
step in the formation of terrestrial planets
8. Binary Star Hypothesis
-proposed that the Sun may have
originally been part of a binary star
system, where two stars orbit a common
center of mass
-the second star was ejected from the
system, leaving our Sun and the planets
in their current configuration
9. The Modern Laplacian Theory
French astronomer and mathematician Pierre-Simon
Laplace first suggested in 1796 that the Sun and the
planets formed in a rotating nebula which cooled and
collapsed
The theory argued that this nebula condensed into
rings, which eventually formed the planets and a central
mass - the Sun
Eventually, after the core has been slowed, its
temperature rises and the dust evaporates
The slowly rotating core becomes the Sun
The faster rotating cloud outside it become the planets
10. The Accretion Theory
The Sun passes through a dense
interstellar cloud
-in a reasonable time the terrestrial
planets form, but the gaseous planets take
far too long to form
The theory does not explain satellites or
Bode's law and is therefore considered the
weakest of those described here
11. Tidal Hypothesis
-suggests that a passing star or another
massive celestial object came close to
the early Sun, causing tidal forces to
disrupt the Sun's outer layers
These ejected materials then coalesced
to form the planets and other objects in
the solar system.
12. The Nebular Hypothesis
proposed by Immanuel Kant and further
developed by Pierre-Simon Laplace in the
18th century
one of the most widely accepted
explanations for the origin of the solar
system
It suggests that the solar system formed
from a giant rotating cloud of gas and dust
called the solar nebula
13. As the nebula contracted and
flattened due to gravity, it began
to spin faster, forming a spinning
disk
In the center, the Sun formed,
and in the outer regions, dust and
gas particles came together to
form planets, moons, asteroids,
14.
15. In 1992 the Hubble Space
Telescope obtained the first
images of proto-planetary disks
in the Orion nebula
They are roughly on the same
scale as the Solar System and
lend strong support to this
16. The Capture Theory
-suggests that the Sun captured already-
formed planets from another star system
-this theory proposes that these planets were
passing through our region of the galaxy, and
the Sun's gravity captured them, causing
them to become part of our solar system
However, this hypothesis is less widely
accepted than the nebular hypothesis
because it's challenging to explain the
composition and orbital characteristics of the