What
is a star??
A star is a luminous
ball of gas, mostly hydrogen and helium, held together by its own gravity.
Nuclear fusion reactions in its core support the star against gravity and
produce photons and heat, as well as small amounts of heavier elements. The Sun
is the closest star to Earth. A star’s color relies on its temperature: hotter
stars emit bluer light and cooler stars emit redder light.
What
is a planet??
According to IAU, an object must
meet three criteria in
order to be classified as a planet.
1. First, it must
orbit the Star.
2. Second, it must be big enough for gravity to squash it
into a round ball.
3. And third, it must have cleared other objects
out of the way in its orbital neighborhood.
What is a galaxy??
A galaxy is a
collection of stars held together by their mutual galaxy. In other words, all
the stars in a galaxy are kept together by the gravity of all the other stars
(as well as the invisible, mysterious dark matter). The best estimates suggest
that the Milky Way contains about 500 thousand million stars.
What
is a comet??
Comets are roving time capsules, carrying
primitive debris from long, long ago.
What
is a satellite??
A natural satellite,
or moon, is a celestial body that orbits another body, e.g. a planet, which is called its primary.
There are 173 known natural satellites
orbiting planets in the Solar
System, as well as at least eight orbiting IAU-listed dwarf planets.
What is a meteor??
A meteor or "shooting star" is the passage of a meteoroid or micrometeoroid into the Earth's atmosphere, incandescent from air friction and shedding glowing material in its wake sufficiently to create a visible streak of light. Meteoroids become meteors when they interact with a
planet's atmosphere and cause a streak of light in the sky.
A
list of planet with number of satellite, distance from sun, a year and a day
measurement is given below:
No.
|
Planet
|
Satellite
|
Distance
|
Orbit
|
Day
|
1
|
Mercury
|
0
|
57
million km
|
88 days
|
58.6 days
|
2
|
Venus
|
0
|
108 million km
|
225 days
|
241 days
|
3
|
Earth
|
1
|
150 million km
|
365.24 days
|
23 hours, 56 minutes
|
4
|
Mars
|
2
|
228 million km
|
687 days
|
24 hours, 37 minutes
|
5
|
Jupiter
|
63
|
779 million km
|
11.9 years
|
9.8 hours
|
6
|
Saturn
|
60
|
1.43 billion km
|
29.5 years
|
10.5 hours
|
7
|
Uranus
|
27
|
2.88 billion km
|
84 years
|
18 hours
|
8
|
Neptune
|
13
|
4.50 billion km
|
165 years
|
19 hours
|
Mercury
The closest planet to the sun, Mercury is
only a bit larger than Earth's moon. Its day side is scorched by the sun and
can reach 840 degrees F (450 C), but on the night side, temperatures drop to
hundreds of degrees below freezing. Mercury has virtually no atmosphere to
absorb meteor impacts, so its surface is pockmarked with craters, just like the
moon.
Discovery: Known to the ancients and visible to the naked
eye
Named for: Messenger of the Roman gods
Venus
The second (2nd) planet from the sun, Venus is terribly
hot. The atmosphere is toxic. The pressure at the surface would crush and kill
you. Scientists describe Venus’ situation as a runaway greenhouse effect. Its
size and structure are similar to Earth, Venus' thick, and toxic atmosphere traps
heat in a runaway "greenhouse effect." Oddly, Venus spins slowly in
the opposite direction of most planets.
The Greeks believed Venus was two different objects — one
in the morning sky and another in the evening. Because it is often brighter
than any other object in the sky — except for the sun and moon — Venus has
generated many UFO reports.
Discovery: Known to the ancients and visible to the naked
eye
Named for: Roman goddess of love and beauty
Earth
The third (3rd) planet from the sun, Earth is a water
world, with two-thirds of the planet covered by ocean. It’s the only world
known to harbor life. Earth’s atmosphere is rich in life-sustaining nitrogen
and oxygen. Earth's surface rotates about its axis at 1,532 feet per second —
slightly more than 1,000 mph — at the equator. The planet zips around the sun
at more than 18 miles per second.
Mars
The fourth (4th) planet from the sun is a cold, dusty
place. The dust, an iron oxide, gives the planet its reddish cast. Mars shares
similarities with Earth: It is rocky, has mountains and valleys, and storm
systems ranging from localized tornado-like dust devils to planet-engulfing
dust storms. It snows on Mars. And Mars harbors water ice. Scientists think it
was once wet and warm, though today it’s cold and desert-like.
Mars' atmosphere is too thin for liquid water to exist on
the surface for any length of time. Scientists think ancient Mars would have
had the conditions to support life, and there is hope that signs of past life —
possibly even present biology
— may exist on the Red Planet.
Discovery: Known to the ancients and visible to the naked
eye
Named for: Roman god of war
Jupiter
The fifth (5th) planet from the sun, Jupiter is huge and
is the most massive planet in our solar system. It’s a mostly gaseous world,
mostly hydrogen and helium. Its swirling clouds are colorful due to different
types of trace gases. A big feature is the Great Red Spot, a giant storm which
has raged for hundreds of years. Jupiter has a strong magnetic field, and with
dozens of moons, it looks a bit like a miniature solar system.
Discovery: Known to the ancients and visible to the naked
eye
Named for: Ruler of the Roman gods
Saturn
The sixth (6th) planet from the sun is known most for its
rings. When Galileo Galilei first studied Saturn in the early 1600s, he thought
it was an object with three parts. Not knowing he was seeing a planet with
rings, the stumped astronomer entered a small drawing — a symbol with one large
circle and two smaller ones — in his notebook, as a noun in a sentence
describing his discovery. More than 40 years later, Christiaan Huygens proposed
that they were rings. The rings are made of ice and rock. Scientists are not
yet sure how they formed. The gaseous planet is mostly hydrogen and helium. It
has numerous moons.
Discovery: Known to the ancients and visible to the naked
eye
Named for: Roman god of agriculture
Uranus
The seventh (7th) planet from the sun, Uranus is an
oddball. It’s the only giant planet whose equator is nearly at right angles to
its orbit — it basically orbits on its side. Astronomers think the planet
collided with some other planet-sized object long ago, causing the tilt. The
tilt causes extreme seasons that last 20+ years, and the sun beats down on one
pole or the other for 84 Earth- years. Uranus is about the same size as
Neptune.
Methane in the atmosphere gives Uranus its blue- green
tint. It has numerous moons and faint rings.
Discovery: 1781 by William Herschel (was thought
previously to be a star)
Named for: Personification of heaven in ancient myth
Neptune
The eighth (8th) planet from the sun, Neptune is known
for strong winds — sometimes faster than the speed of sound. Neptune is far out
and cold. The planet is more than 30 times as far from the sun as Earth. It has
a rocky core. Neptune was the first planet to be predicted to exist by using math,
before it was detected. Irregularities in the orbit of Uranus led French
astronomer Alexis Bouvard to suggest some other might be exerting a gravitational
tug. German astronomer Johann Galle used calculations to help find Neptune in a
telescope. Neptune is about 17 times as massive as Earth.
Discovery: 1846
Named for: Roman god of water
Pluto
It is unlike other planets in many respects. It is smaller
than our moon. Its orbit carries inside the orbit of Neptune and the way out
beyond that orbit. From 1979 until early 1999, Pluto had actually been the eighth
planet from the sun. Then, on Feb. 11, 1999, it crossed Neptune's path and once
again became the solar system's most distant planet — until it was demoted to
dwarf planet status. Pluto will stay beyond Neptune for 228 years. Pluto’s
orbit is tilted to the main plane of the solar system — where the other planets
orbit — by 17.1 degrees. It’s a cold, rocky world with only a very ephemeral
atmosphere.
Discovery: 1930 by Clyde Tombaugh
Named for: Roman god of the underworld, Hades
The
problem for Pluto
The problem for Pluto is the fact
that its orbit is in the Kuiper Belt along with 43 other known Kuiper Belt
Objects (KBOs). There are possibly billions of objects in the Kuiper Belt that
have not been cataloged yet. Scientists have even found 8 KBOs between Neptune
and Pluto. Some scientists view the new definition as unclear. Exactly how much
does Pluto have to "clear" from its neighborhood to be considered a
planet? And how much has Pluto already influenced its own neighborhood since
the planet formed? These and other questions have been raised in response to
the IAU's definition of a planet.
Consider this: Pluto crosses into
Neptune's orbit, but Neptune is still classified a planet. This is because of
the orbits of Pluto and Neptune and that they never get closer to each other
than 17AU (AU=distance from Earth to the Sun). Pluto may cross orbits with many
other Kuiper Belt Objects, but how close do these objects get to Pluto? How
close to objects have to get to Pluto to be considered "in" Pluto's
neighborhood? Diagram of the planet orbits in our solar system, including
Pluto, distinctly shows the crossover of Neptune's and Pluto's orbits.
sources:
wikipedia.com
nasa.gov
space.com
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