We in the U N I V E R S E
Blog #11
The Solar Family
Abstracts:
Milky Way, a part of Galaxy,
consists of millions of stars including our Sun. Most of the stars have their
family, but some do not have. Our Sun has its family known as the Solar System, which comprises of many major,
and minor planets, their satellites, dwarf planets, comets, asteroids and
meteoroids. These all work in a systematic order. Its formation has taken a
long series of very complex processes. In every moment, many stars are created
as well as destroyed. Our Sun will also be destroyed after completing its life
in billions of years ahead. However, in different age of life of the Sun, the
solar family and its every member behave in different manner and finally they all
shall contained back into the Sun.
Introduction
The Solar System is the
gravitationally bounded system of the Sun and the objects within. The largest
of them are the eight planets, namely Mercury, Venus, Earth, Mars, Jupiter,
Saturn, Uranus, and Neptune divided into two groups of four planets in each
group, known as the inner planets (includes Mercury, Venus, Earth and Mars) and
the outer planets (includes Jupiter, Saturn, Uranus and Neptune). The eight
planets in order from the sun are four terrestrial planets, also called the
inner planets; the two gas giants, Jupiter and Saturn; and two ice giants,
Uranus and Neptune. The formation of Solar System Considered to be initiated
about 4.6 billion years ago when a dense region of a molecular cloud collapsed,
forming the sun and a protoplanetary disk.
Some important facts about
the Solar system
Age: 4.568 billion years
approximately
Stars: 1 (Sun)
Known natural satellites: 758 (285 planetary, 473
minor planetary)
Known minor planets: 7,298,470
Known comets: 4,586
Identified rounded
satellites:
19
Known planets:
Mercury, Venus, Earth,
Mars, Jupiter, Saturn, Uranus, and Neptune.
Known dwarf planets:
Ceres, Pluto, Haumea,
Quaoar, Makemake, Gonggong, Eris and Sedna.
Location:
local interstellar cloud,
local bubble, Orion- Cygnus Arm, Milky Way
Nearest star: a) Proxima Centauri (4.2465 light years) and
b) Alpha Centauri (4.344 light years)
Nearest
planetary system: Proxima Centauri System
The Solar Family:
According to the available data, about 4.6 billion years ago,
our sun came into existence, and with time, it created its own family of
planets, comets, asteroids, meteoroids and other entities. The planets which
are a part of the solar system were formed from the gaseous clouds and dust
that remained after the Sun was formed. The planets started to take shape
around 4.6 billion years ago i.e. along with the formation of Sun. Some of the
dust, pieces of rock and gas particles which were orbiting the Sun smashed
against each other and began to heat up until the entire mass melted. As the
mass grew, it began large enough to create its own magnetic force and gravity.
The force kept the materials safe from flying off into the space again. It also
attracted more materials, until the area around became free of debris and the
planets started to get its shape. Some materials in this mass that were heavier
than others fell towards the center of the mass to become the core. The rest
formed the upper layers towards surface likewise, according to their masses and
density. The round shape of the planets and other objects took place due to its
circular motion on its own axis. All the planets in this solar system were
formed in this manner, about one hundred and thirty million years ago; in the
same way the planet’s satellites also came into existence. We named the planets
of the Solar System as Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and
Neptune. Notably, Pluto was considered as a planet earlier; notwithstanding its
rotational path, it has been removed from the list of planets in year 2006 and
is now considered as a dwarf planet (The detailed reason of this removal shall
be discussed later in this chapter).
The four terrestrial planets having solid surface, belong to
the inner solar system. Inversely, all the four giants belong to the outer
Solar System; and they do not have any definite surface, as they are mainly
composed of gases and liquids. Interestingly, 99.86% mass of the solar system is
contained in the Sun alone. in the remaining part, 90% of the mass is fulfilled
by the combined mass of the Jupiter and Saturn. There is a strong consensus
among astronomers that the solar system also has eight dwarf planets, which
consists of one asteroid belt object Ceres, four Kuiper belt objects, Pluto,
Haumea, Quaoar and Makemake and three scattered disc objects: Gonggong,
Eris and Sedna.
Solar Family: A Fact File
Planets visible to naked eyes: Mercury, Venus, Earth, Mars and
Jupiter.
Great planets/super giants: Jupiter, Saturn, Uranus and
Neptune.
Inferior planets: Mercury and Venus
Terrestrial planets: Mercury, Venus, Earth and Mars
Some Important Definitions
Comets
A comet is the cosmic snowball of frozen gases, rock and dust
that orbits the sun. When frozen, these are the size of a town. When a comet’s orbit
brings it close to the sun, it heats up and spews dust and gases into a giant
glowing head larger than most planets.
Asteroids
An asteroid is a minor planet- an object that is neither a
true planet nor a comet, but orbits within the inner solar system. They are
rocky, metallic or icy bodies with no atmosphere.
Meteoroids
A meteoroid is a small rocky or metallic body in the outer
space. Meteoroids are distinguished as objects significantly smaller than
asteroids, ranging in size from grains to objects up to a meter wide. Objects
smaller than the meteoroids are called micrometeoroids
or space dust.
Planetary
System
It
is a set of gravitationally bound non stellar objects in or out of orbit around
a star or a Star’s family system. Generally speaking, systems with one or more
planets constitute a planetary system, although such systems may also consist
of bodies such as dwarf planets, asteroids, natural satellites, meteoroids,
comets, planetesimals and circumstellar discs.
Planetesimals
The minute planets which are under formation of a planet along
with many other entities under gravitation.
Circumstellar discs
After a star is formed, the remaining dust and gas is
trapped in orbit, forming a rotating disc or torus around the young star.
Terrestrial
Planets
The first four planets from the Sun; i.e. Mercury, Venus,
Earth and Mars. These planets are mainly composed of rocks and metals. These
planets are also known as inner planets.
Provisional Moons
Moons under assumption or research are kept under the
category of provisional moons. However, they will be given a proper name when
their discoveries are confirmed by additional observations.
Rounded
Satellites
All
the other known satellites that are at least the size of Uranus’ Miranda have
lapsed into rounded ellipsoids under hydrostatic equilibrium, i.e. they are
‘round satellites’ or ‘rounded satellites’ and are sometimes categorized as the
planetary mass moons.
Dwarf
planets
A dwarf planet is a small planetary- mass object that directly
orbits around the sun, and massive enough to have gravitationally rounded, but
is insufficient to achieve an orbital dominance like the eight planets in the
solar system. The prototypical dwarf planet is Pluto, which was regarded as the
planet before the ‘dwarf planet’ concept was adopted in 2006.
The term ‘dwarf planet’ was coined by a planetary scientist: Alan
stern as part of a three-way categorization of planetary mass objects in the
solar system. Classical planets, dwarf planets and satellite planets. Dwarf
planets were thus conceived of as a category of planet. In 2006, however, the
concept was adopted but the International Astronomical Union (IAU) as a
category of planet and sub planetary objects, part of a three-way re-categorization
of bodies orbiting the Sun: planets, dwarf planets and small solar system
bodies. Thus Stern and other geologists consider dwarf planets and large
satellites to be planets, but since 2006, the IAU and perhaps the majority of
astronomers have excluded them from the list of planets.
The interest of dwarf planets to planetary geologists is that
they may be geologically active bodies, an expectation that this concept was
borne out in 2015 by the Dawn mission to Ceres and New Horizons mission to Pluto. Astronomers are in general
agreement that at least the eight largest candidates are the dwarf planets- in
irregular order of size: Pluto, Eris,
Haumea, Makemake, Gonggong, Quaoar, Sedna and Ceres.
Natural
Satellites or Satellites
A natural satellite is in the most common usage, an
astronomical body that orbits a planet, dwarf planet, small solar system body
or even in some cases; found to orbit around another natural satellite. Natural
satellites are colloquially referred to as moons, a derivation from the moon of
earth. In our Solar System, there are six planets having at least one moon;
with altogether it contains two hundred and eighty-four (284) known natural
satellites. Seven objects which are commonly considered as dwarf planets by the
astronomers are also known to have natural satellites. These dwarf planets are Pluto, Haumea, Makemake, Gonggong, Salacia,
Quaoar and Eris. As per the
studies of November 2021, there are four hundred and forty-two (442) other
minor planets in the Solar System known to have natural satellites.
A planet is at least ten thousand (10,000) times heavier by
the mass of its any of the natural satellite(s). The Earth and Moon system in
the Solar System is a unique exception. The diameter of the Moon is 0.273 times
the diameter of the Earth. The mass of the Earth is 80 times the mass of the
moon. The next larger ratios are the Neptune and Trion system at 0.055, the
Saturn and Titan system at 0.044, the Jupiter and Ganymede system at 0.031. For
the dwarf planet category, Charon has the highest ratio being 0.52 the diameter
and 12.2% of the mass of Pluto.
Planets
A planet is a large, rounded, astronomical body that is
neither a star nor its remnant. But best available theory of planet formation is
the nebular
hypothesis, which posits an
interstellar cloud collapses out of a nebula to create a young protostar
orbited by a protoplanetary disk. Planets grow in this disk by the gradual
accumulation of material driven by gravity, a process called accretion. The
Solar System has at least eight planets, the terrestrial as well as the giant
ones.
The word planet comes from the Greek word Planetai which means wandering. In
antiquity, this word refers to the sun, moon and five points of the light
visible to the naked eye that moved across the background of the stars- namely:
Mercury, Venus, Mars, Jupiter and Saturn. Planets have historically had
religious associations, multiple cultures identified celestial bodies with Gods,
and these connections with mythology and folklore persists in the schemes for
naming the newly discovered solar system bodies. Earth itself is recognized as
a planet when heliocentric theory replaced the geocentric theory in the 16th
and 17th century.
With the discovery and further development of the telescope,
the meaning of planet broadened to include only visible with assistance, the
moons of the planets beyond earth; the ice giants- Uranus and Neptune, Ceres
and other bodies, later recognized to be a part of the asteroid belt. And then Pluto, found to be the largest member of
the collection of icy bodies known as the Kuiper
Belt. The discovery of other large objects in the Kuiper Belt, particularly
Eris, spurred debate about how exactly to define a planet.
The Indian Astrological theory suggests the nine planets (Sun,
Moon, Mars, Mercury, Jupiter, Venus, Saturn, Uranus and Neptune) other than Earth
which includes all the eight planets of the solar system, based on the theory
of Geocentric Arrangement. Theory was established in the post Vedic Age,
thousands of years ago. However, the details about the physical being and
nature of the planets along with its rotational data and distance from the
earth are identical to the data produced by the modern researches.
An overview
of the Planets of the Solar System:
Mercury:
Distance from the Sun: 57,909,227 Kilometers
Equatorial Diameter: 4,879.40 Kilometers
Mass: 3.30 X 1020 Tones
Density: 5.43 times that of water
Surface temperature: -173 degree Celsius to +427 degree
Celsius
Period of Rotation: 58 days 15 hours 30 minutes
Revolution around the Sun: 87 days 23 hours 17 minutes
Number of known Moons: 0
Venus
Distance from the Sun: 108,209,475 Kilometers
Equatorial Diameter: 12,103.61 Kilometers
Mass: 4.87 X 1021 Tones
Density: 5.24 times that of water
Surface temperature: +462 degree Celsius
Period of Rotation: 243 days 26 hours
Revolution around the Sun: 224 days 16 hours 48 minutes
Number of known Moons: 0
Earth
Distance from the Sun: 149,598,262 Kilometers
Equatorial Diameter: 12,742 Kilometers
Mass: 5.97 X 1021 Tones
Density: 5.51 times that of water
Surface temperature: -88 degree Celsius to +58 degree
Celsius
Period of Rotation: 23 days 56 hours
Revolution around the Sun: 1 year (365 days 6 hours14 minutes)
Number of known Moons: 1
Mars
Distance from the Sun: 227,943,824 Kilometers
Equatorial Diameter: 6,779 Kilometers
Mass: 6.42 X 1020 Tones
Density: 3.93 times that of water
Surface temperature: -87 degree Celsius to -5 degree
Celsius
Period of Rotation: 1 day 37 hours
Revolution around the Sun: 1 year 321 days 37 hours
Number of known Moons: 2
Jupiter
Distance from the Sun: 778,340,821 Kilometers
Equatorial Diameter: 139,822 Kilometers
Mass: 1.90 X 1024 Tones
Density: 1.33 times that of water
Surface temperature: -148 degree Celsius
Period of Rotation: 9 hours 55 minutes
Revolution around the Sun: 11 years 314 days 20 hours
Number of known Moons: 66 (out of 66, 16 are provisional
moons)
Saturn
Distance from the Sun: 1,426,666,422 Kilometers
Equatorial Diameter: 116,464 Kilometers
Mass: 5.68 X1023 Tones
Density: 0.70 times that of water
Surface temperature: -178 degree Celsius
Period of Rotation: 10 hours39 minutes
Revolution around the Sun: 29 years 163 days 8 hours 5 minutes
Number of known Moons: 62 (out of 62, 9 are provisional
moons)
Uranus
Distance from the Sun: 2,870,658,186 Kilometers
Equatorial Diameter: 50,724 Kilometers
Mass: 8.68 X 1022 Tones
Density: 1.30 times that of water
Surface temperature: -216 degree Celsius
Period of Rotation: 17 hours 14 minutes
Revolution around the Sun: 84 years 6 days 3 hours 34 minutes
Number of known Moons: 27
Neptune
Distance from the Sun: 4,498,396,441 Kilometers
Equatorial Diameter: 49,244 Kilometers
Mass: 1.02 X 1023 Tones
Density: 1.64 times that of water
Surface temperature: -214 degree Celsius
Period of Rotation: 16 hours 7 minutes
Revolution around the Sun: 164 years 288 days 50 minutes
Number of known Moons: 13
Pluto:
No Planet Anymore…
According to the definition set by the IAU, a planet must have
its own separate orbit; but Pluto did not have any orbit of its own. In its
every orbital cycle of 248 years, it gradually enters in the orbit of the
Neptune remains 20 years in that orbit and then comes out to its original path
i.e. it intercepts the orbit of Neptune which implies that it does not have its
own independent orbit and it is a primary condition for an entity to be a
planet. Therefore, its name was ousted from the list of planets in 2006.
Lastly, Pluto was roaming in the orbit of the Neptune from 7th
February 1979 to 11th February 1999.
Table 1: showing the distance from
the Sun, number of moons, temperature, number of rings and relative mass to
Earth of the planets of the solar system.
Planet |
Distance from Sun (EU) |
Number of Moons |
Temperature in Celsius |
Rotational period |
Mercury |
0.39 |
0 |
-170 to 390 |
58d15h36m |
Venus |
0.72 |
0 |
475 |
243 d |
Earth |
1.0 |
1 |
22 |
23h56m |
Mars |
1.52 |
2 |
-23 |
24h37m |
Jupiter |
5.2 |
16 |
-123 |
10h |
Saturn |
9.54 |
22 |
-180 |
10h40m |
Uranus |
19.2 |
15 |
-218 |
16h |
Neptune |
30.1 |
2 |
-228 |
18h |
EU = Earth Unit; d days, h hours, m minuts.
Table 2: showing the color, orbital speed, rotation period
and orbital period of the planets of the solar system.
Planets |
No. of
Rings |
Relative
Mass |
Color |
Orbit speed |
Orbit period |
Mercury |
0 |
0.06 |
M&E
Str |
47.9 |
88d |
Venus |
0 |
0.82 |
M&E
Str |
35 |
224.7d |
Earth |
0 |
1 |
Blue |
29.8 |
365.2d |
Mars |
0 |
0.11 |
Red |
24.1 |
1.88y |
Jupiter |
1 |
318 |
Red spot |
13.1 |
11.86y |
Saturn |
Ex Sys |
95 |
Blackish |
9.6 |
29.46y |
Uranus |
10 |
15 |
Green |
6.8 |
84y |
Neptune |
1 |
17 |
Greenish |
5.4 |
164.8y |
M&E Str = Morning and
evening Stars
Terminology:
The first known natural satellite was the Moon, but it was
considered as a planet until Copernicus, introduced his De revolutionibus orbium coelestium in 1543. Until the discovery of
the Galilean satellites in 1610, there was no opportunity for referring to such
objects as a class. The first to use the term satellite to describe the
orbiting bodies was the German Astronomer Johannes Kepler. He described the
orbiting bodies in his pamphlet Narratio
de Observatis a se quator louis satellitibus erronibus (Narration About
Four Satellites of Jupiter Observed) in 1610. He derived the term from the
Latin word Satelles, meaning ‘guard’,
‘attendant’ or ‘companion’ because the satellites accompanied their primary planet
throughout their journey.
Conclusion:
Our Sun has a very rich and interesting
story about its formation and creation of the Solar Family. We are fortunate to
be a part of our Solar Family as it is rear combination of the matters,
atmosphere and environment support life. The nearest stars are the Proxima
Centauri with its family, called the Proxima
Centauri System and Alpha
Centauri without family. The eight planets which orbit around the sun are known
as the major planets, whereas some other minor planets are also roaming and
revolving inside the solar system.
Sun is responsible to hold on the entire
Solar family to posit its situation and source of energy for the functions of
all the terrestrial activities as well as the existence of the life anywhere
within. This is why Sun is tribute to be the father of the whole Solar family
system.
Total words: 3000+
Sources of Data:
Wikipedia
Space.com
Amnh.com
Study.com
Science.nasa.gov
Google and other websites
Orient Blackswan School Atlas
Other course materials
Manorama Tell Me Why Earth
Vedanta
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