How Do Greenhouse Gases Actually Work?

How Do Greenhouse Gases Actually Work?

# The Temperature Difference between Earth and Moon

This section explains the temperature difference between the Earth and the Moon, despite being at similar distances from the Sun.

Temperature Variation on the Moon

  • The average temperature on the Moon is -18°C, ranging from -170°C during lunar night to 100°C at lunar noon.
  • These temperatures exceed both the coldest and hottest temperatures ever recorded on Earth.
  • The duration of days and nights on the Moon is about 14 times longer than on Earth.

Role of Earth's Atmosphere

  • The Earth's atmosphere protects us from extreme temperatures.
  • During daytime, it acts as a shield, blocking harmful solar rays and one-third of visible light.
  • At night, it traps infrared radiation (heat) radiating from the Sun-warmed surface, preventing freezing.

Electrically-Charged Particles in Atmosphere

  • For an atmosphere to absorb radiation, it needs electrically charged particles for electromagnetic waves to interact with.
  • Most of our atmosphere consists of gas molecules without an electric charge.
  • However, some molecules have a lopsided distribution of negatively-charged electrons that can absorb energy from incoming infrared rays.

Infrared Absorption by Lopsided Molecules

  • Molecules like water, ozone, and nitrous oxide are electrically lopsided and can absorb infrared radiation.
  • Carbon dioxide and methane molecules may not appear lopsided but their motion causes them to vibrate in electrically-lopsided ways, allowing them to absorb infrared rays.

Majority of Atmosphere Cannot Absorb Infrared Radiation

  • Nitrogen and oxygen make up most of our atmosphere but they do not get lopsided even when vibrating due to their symmetric structure.
  • However, the lopsided 1% of molecules in our atmosphere are excellent infrared absorbers. They intercept about 90% of Earth's outgoing heat.
  • These absorbed rays get bounced around the atmosphere and often return to the surface before escaping to space.

# Importance of Radiation-Pinball Game for Earth

This section highlights the significance of the radiation-pinball game in regulating Earth's temperature.

Impact of Atmospheric Carbon Dioxide

  • Ice records from Earth's coldest climate show that small variations in atmospheric carbon dioxide lead to significant temperature changes.
  • Compared to the last 800,000 years, today's game of regulating temperature is much more challenging.

# Acknowledgements

The video acknowledges the team at Kurzgesagt for their animations and invites viewers to check out their channel.

Collaboration with Kurzgesagt

  • The video expresses gratitude to the team at Kurzgesagt for creating the animations.
  • Viewers are encouraged to visit Kurzgesagt's channel, which covers a wide range of topics from neutron stars to fracking and Islamic culture.

Timestamps have been associated with relevant sections as per the transcript provided.

Video description

Thanks to Kurz Gesagt for illustrating this video! http://www.youtube.com/kurzgesagt And for composing the music!: https://soundcloud.com/epicmountain/minute-earth Thanks also to our Patreon patrons: - AshrafDude - Nasser Hamed Alminji - Jeff Straathof - Mark - Maarten Bremer - Today I Found Out - Avi Yashchin - Valentin - Nicholas Buckendorf - @AntoineCoeur And our Subbable Sponsors: - Tori McClanahan - Evan Gale - Ho Yin Michael Cheng - http://lovescomputers.com/ - Raymond Cason - Shalom Craimer - Nick Pietrzak - TPRJones - http://i3.kym-cdn.com/photos/images/newsfeed/000/002/941/Duckroll.jpg - @Lexify - @Asajii - Robin S. - https://code.org/ - Nicholas Buckendorf - Alison G. - choklitfroggie.tumblr.com - Cameron Johnson - Tom Headley - https://www.etsy.com/shop/Piecesofgame - @thenarcolepsist - Bas Hessels - http://bashessels.nl - Nauda Family - Danielle Lane ___________________________________________ Want to learn more about the topic in this week’s video? Here are some key words/phrases to get your googling started: - Radiation balance - incoming radiant energy from the sun minus outgoing energy heading into space. - Infrared radiation - electromagnetic radiation that is invisible to us; comes in longer wavelengths than visible light and provides energy transfer we call heat. ________________________ MinuteEarth provides an energetic and entertaining view of trends in earth’s environment – in just a few minutes! Subscribe on YouTube: http://www.youtube.com/user/minuteearth?sub_confirmation=1 Created by Henry Reich With the MinuteEarth team: Alex Reich, Peter Reich, Emily Elert, Ever Salazar, Kate Yoshida, and Henry Reich. Music by Nathaniel Schroeder: http://www.soundcloud.com/drschroeder ________________________ Please support us on Patreon: https://www.patreon.com/minuteearth And follow us on Vessel: https://www.vessel.com/shows/6891774506155638 And here we are on iTunes: https://goo.gl/sfwS6n Also, say hello on: Facebook: http://facebook.com/minuteearth Twitter: http://twitter.com/MinuteEarth ________________________ References: Virtual Chembook, Elmhurst College, Charles E. Ophardt http://elmhcx9.elmhurst.edu/~chm/vchembook/globalwarmA5.html Climate and Earth’s Energy Budget, NASA Earth Observatory http://earthobservatory.nasa.gov/Features/EnergyBalance/page6.php Infrared spectroscopy/Caltech (mirrored from UCLA chemistry) http://www.wag.caltech.edu/home/jang/genchem/infrared.htm http://elmhcx9.elmhurst.edu/~chm/vchembook/globalwarmA5.html