ALIEN INTERVIEW - THE NEW EARTH - Earth Changes and The ...

One megalight-year, abbreviated "Mly", is one million light-years, or about 306,600 parsecs.
Megalight-years are typically used to measure distances between neighboring galaxies and
galaxy clusters.
One gigalight-year, abbreviation "Gly", is one billion light-years — one of the largest distance
measures used. One gigalight-year is about 306.6 million parsecs.
-- Reference: Wikipedia.org
211 "... a heavy gravity, nitrogen/oxygen atmosphere planet..."
"The Earth's atmosphere is a layer of gases surrounding the planet Earth and retained by
the Earth's gravity. It contains roughly (by molar content/volume) 78.08% nitrogen, 20.95%
oxygen, 0.93% argon, 0.038% carbon dioxide, trace amounts of other gases, and a variable
amount (average around 1%) of water vapor. This mixture of gases is commonly known as
air. The atmosphere protects life on Earth by absorbing ultraviolet solar radiation and
reducing temperature extremes between day and night.
There is no definite boundary between the atmosphere and outer space. It slowly becomes
thinner and fades into space. Three quarters of the atmosphere's mass is within 11 km of the
planetary surface. In the United States, people who travel above an altitude of 80.5 km (50
statute miles) are designated astronauts. An altitude of 120 km (~75 miles or 400,000 ft)
marks the boundary where atmospheric effects become noticeable during re-entry. The
Kármán line, at 100 km (62 miles or 328,000 ft), is also frequently regarded as the boundary
between atmosphere and outer space.
The atmosphere of Mars is relatively thin, and the atmospheric pressure on the surface
varies from around 30 Pa (0.03 kPa) on Olympus Mons's peak to over 1155 Pa (1.155 kPa)
in the depths of Hellas Planitia, with a mean surface level pressure of 600 Pa (0.6 kPa),
compared to Earth's 101.3 kPa. However, the scale height of the atmosphere is about
11 km, somewhat higher than Earth's 6 km. The atmosphere on Mars consists of 95%
carbon dioxide, 3% nitrogen, 1.6% argon, and contains traces of oxygen, water, and
methane. The atmosphere is quite dusty, giving the Martian sky a tawny color when seen
from the surface; data from the Mars Exploration Rovers indicates the suspended dust
particles are roughly 1.5 micrometres across.
The atmosphere of Venus, the second planet from the Sun, is much denser and hotter than
that of Earth. The surface temperature and pressure on Venus are 740 K (467°C) and
93 bar, respectively. The Venusian atmosphere supports thick persistent clouds made of
sulfuric acid, which make optical observations of the surface impossible. The information
about surface features on Venus has been obtained exclusively by radar imaging conducted
from the ground and Venera 15-16 and by Magellan space probes. The main atmosphereric
gases on Venus are carbon dioxide and nitrogen, which make up 96.5% and 3.5% of all
molecules. Other chemical compounds are present only in trace amounts.
The atmosphere of Venus is in state of a vigorous circulation and super-rotation. The whole
atmosphere circles the planet in just four days (super-rotation), which is a short time
compared with the sideral rotational period of 243 days. The winds supporting super-rotation
blow as fast as 100 m/s. Near the poles of Venus anticyclonic structures called polar
vortexes are located. In them the air moves downward. Each vortex is double eyed and
shows a characteristic S-shaped pattern of clouds.
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