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2. Atmosphere of Earth - Wikipedia

   en.wikipedia.org/wiki/Atmosphere_of_Earth

   The atmosphere has a mass of about 5.15 × 10 18 kg, [4] three quarters of which is within about 11 km (6.8 mi; 36,000 ft) of the surface. The atmosphere becomes thinner with increasing altitude, with no definite boundary between the atmosphere and outer space. The Kármán line, at 100 km (62 mi) or 1.57% of Earth's radius, is often used as ...

3. All Dogs Go to Heaven 2 - Wikipedia

   en.wikipedia.org/wiki/All_Dogs_Go_to_Heaven_2

   Box office. $8.6 million [1] All Dogs Go to Heaven 2 is a 1996 American animated musical fantasy adventure film, and a sequel to Goldcrest Films ' animated film All Dogs Go to Heaven (1989). [2] Produced by MGM/UA Family Entertainment and Metro-Goldwyn-Mayer Animation, it was co-directed by Paul Sabella and Larry Leker.

4. Earth's energy budget - Wikipedia

   en.wikipedia.org/wiki/Earth's_energy_budget

   Earth's energy imbalance (EEI) Earth's energy budget (in W/m 2) determines the climate. It is the balance of incoming and outgoing radiation and can be measured by satellites. The Earth's energy imbalance is the "net absorbed" energy amount and grew from +0.6 W/m 2 (2009 est. [8]) to above +1.0 W/m 2 in 2019. [23]

5. Earth - Wikipedia

   en.wikipedia.org/wiki/Earth

   Earth is the third planet from the Sun and the only astronomical object known to harbor life. This is enabled by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all of Earth's water is contained in its global ocean, covering 70.8% of Earth's crust.

6. Earthrise - Wikipedia

   en.wikipedia.org/wiki/Earthrise

   Earthrise, taken on December 24, 1968, by Apollo 8 astronaut William Anders. Earthrise is a photograph of Earth and part of the Moon 's surface that was taken from lunar orbit by astronaut William Anders on December 24, 1968, during the Apollo 8 mission. [1] [2] [3] Nature photographer Galen Rowell described it as "the most influential ...

7. Future of Earth - Wikipedia

   en.wikipedia.org/wiki/Future_of_Earth

   The Sun will experience more rapid mass loss, with about 33% of its total mass shed with the solar wind. The loss of mass will mean that the orbits of the planets will expand. The orbital distance of Earth will increase to at most 150% of its current value (that is, 1.5 AU (220 million km; 140 million mi)).