Venus
Hii , welcome to my post . Today we are going to know about Venus (planet). So let's start :
Definition:
• Venus is the second planet from the Sun.
• It is sometimes called Earth's "sister" or "twin" planet.
• It is almost as large and has a similar composition
like Earth.
appears in Earth's sky, either as morning Star or
evening star.
• Aside from the Sun and Moon, Venus is the brightest
natural object in Earth's sky.
• It is capable of casting visible shadows on Earth at
dark conditions.
• It is being visible to the naked eye in broad daylight.
• Venus is one of the four inner terresterial planets.
Facts :
• Venus was the first planet explored by a spacecraft.
• It was intensely studied early in the history of space
exploration.
• Venus was also the first planet whose surface was
reached by a spacecraft from Earth.
• The intense heat means landers have only survived
for a couple of hours.
• Venus rotates backward on its axis compared to most
planets in our solar system.
• This means the Sun rises in the west and sets in the
east, opposite of what we see on Earth.
• Venus is an unlikely place for life as we know it, but
some scientists theorize microbes might exist high in
the clouds where it’s cooler and the pressure is
similar to Earth’s surface. Phosphine, a possible
indicator of microbial life, has been observed in the
clouds.
• Venus rotates very slowly on its axis – one day on
Venus lasts 243 Earth days.
• The planet orbits the Sun faster than Earth, however,
so one year on Venus takes only about 225 Earth
days, making a Venusian day longer than it.
Quick Facts :
Mass (1024kg)------- 4.87
Diameter (km)------ 12
Density (kg/m3)------- 5243
Gravity (m/s2)------ 8.9
Escape Velocity (km/s)---- 10.4
Rotation Period (hours)------ 5832.5
Length of Day (hours)------ 2802
Aphelion (106 km)----- 108.9
Orbital Period (days)------- 224.7
Orbital Velocity (km/s)------ 35
Orbital Inclination (degrees)------- 3.4
Orbital Eccentricity------- 0.007
Obliquity to Orbit (degrees)------ 177.4
Mean Temperature (C)----- 464
Surface Pressure (bars)-------- 92
Composition:
• Venus has a thick, toxic atmosphere filled with carbon
dioxide.
• Venus has an extremely dense atmosphere
composed of 96.5% carbon dioxide, 3.5% nitrogen—
both exist as supercritical fluids at the planet's
surface.
• It’s perpetually shrouded in thick, yellowish clouds of
sulfuric acid that trap heat, causing a runaway
greenhouse effect.
• It’s the hottest planet in our solar system, even
though Mercury is closer to the Sun.
• Surface temperatures on Venus are about 900
degrees Fahrenheit (475 degrees Celsius) – hot
enough to melt lead.
• The surface is a rusty color and it’s peppered with
intensely crunched mountains and thousands of
large volcanoes.
• Venus has a solid surface covered in dome-like
volcanoes, rifts, and mountains, with expansive
volcanic plains and vast, ridged plateaus.
Structure:
• Venus is not a gas planet, but a rocky planet.
• Mainly structure of Venus consists of Crust, Mantle,
and Core.
(i) Crust :
• Venus' crust is mostly basalt and is estimated to
be 6 to 12 miles (10 to 20 km) thick.
(ii) Mantle :
• Venus' molten rocky mantle is roughly 1,200 miles
(3,000 km) thick.
(iii) Core :
• The interior of Venus is made of a metallic iron
core that's roughly 2,400 miles (6,000 km) wide.
Thankyou
In this post i have given information only about Venus (planet). The other parts of Solar system will be described in further posts .
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