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Tag Archives: atmosphere

Falling Sky: China’s Tiangong 1 Space Station Last Hours

28 Wednesday Mar 2018

Posted by Paul Kiser in About Reno, All Rights Reserved, Astronomy, China, Exploration, NASA, Reno, Science, Space, Technology

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atmosphere, China, Chinese Space Agency, deorbit, ISS, orbit, Skylab, Space Station, Tiangong 1

Within the next 72 hours China’s first space station, the Tiangong 1, is going to end its life. It is already scraping the extreme upper atmosphere of Earth and the air resistance is slowing down the 7.7 metric tons (8.5 ton) spacecraft with every passing second. It is coming down somewhere, but scientists don’t know exactly when or where.

Tiangong altitude

The rapid altitude decline (in km) of Tiangong 1

Current Stats of Tiangong 1

The current speed of the Tiangong 1 (27 March 2018 at 12 noon PDT) is at 28,000 km/hr (17,400 mph) and it is at an altitude of just under 200 km (125 mi) at the lowest point in its orbit. Its orbit has lowered by over 60 km in the last two months. As Tiangong 1 approaches 160 km the air resistance will be too much for it to maintain orbit.

Statistically, Tiangong 1 will most likely fall into an ocean; however, there is a possibility that it could fall on southern Europe, southern Asia, Africa, Austrailia, South America, Central America, or the United States.

Lost Contact

Normally, objects like this are brought down in a controlled fall using thrusters to slow the craft down at a specific time and location. In the case of Tiangong 1, the Chinese engineers had planned to bring it down in a controlled reentry until they mysteriously lost contact with it two years ago.

China said they had shut down telemetry with Tiangong 1 in March of 2016. They didn’t admit they had lost control of it until amateur astronomers had confirmed the space station was tumbling in space a few months later. Without the ability to communicate with the space station, there is no way to command the thrusters for a controlled reentry.

Best Guess?

The experts are currently estimating that Tiangong 1 will come down on Easter Sunday (1 April.) Since Earth’s atmosphere expands and contracts with solar activity, the air resistance is not consistent. There is a critical point when the air resistance will win its battle with the space station and the orbit will decay exponentially. At that point, the spacecraft will begin a rapid breakup as it descends through the thicker atmosphere.

For what it’s worth, my guess is 7:42 am PDT on Saturday, 31 March.

Can Venus Be Made Habitable?

25 Monday Dec 2017

Posted by Paul Kiser in Green, Science, solar, Space, Technology, Travel

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atmosphere, carbon dioxide, CO₂, CO², Earth, extreme makeover, Global warming, greenhouse effect, hydrogen, nitrogen, O², oxygen, solar system, terraforming, Venus, Weather

Venus: Too hot, too much atmosphere

Venus may be the future of Earth and may also hold the answers to global warming.

Earth’s atmosphere is 78 percent nitrogen, 21% oxygen, (O₂,) and 1% other gases including carbon dioxide (CO₂) and water vapor. Even though CO₂ is considered a trace gas in our atmosphere it is a major player in the absorption of energy from the Sun. Nitrogen and oxygen are ‘invisible’ to the Sun’s radiation, so the energy from the Sun passes through the two gases without being absorbed.

The atmosphere of Venus 96% CO₂ and 3.5% nitrogen, with 0.5% other gases, including water vapor. Venus’ atmosphere is also extremely dense. The pressure at the surface of Venus is the same as the pressure at 1,000 meters (3,000 ft.) under the surface of Earth’s ocean.

Venus is also hot. The CO₂ absorbing the Sun’s energy retains the heat in a runaway greenhouse effect that keeps the temperature at 462 °C (864 °F,) both day and night.

The interesting, and terrifying fact is that the carbon found on Earth is roughly equal to the carbon found on Venus. The difference is that Earth stores its carbon in the ocean, and in calcite deposits that consists of dead marine life that settled in the bottom of an ocean and became a sedimentary rock formation.

There is also a nitrogen problem. Even though nitrogen makes up 3.5% of Venus’ atmosphere, it is four times the amount of nitrogen in Earth’s atmosphere.

Venus could be Earth Like if:

  • Almost all of the atmospheric carbon and three-quarters of the nitrogen could be transformed into solid carbon and solid nitrogen.
  • Some of the oxygen from the CO₂ could be liberated for the atmosphere.
  • The rest of the oxygen could be liberated to combine with hydrogen in the upper atmosphere to create water.
  • The Sun’s energy could be reduced (blocked) to allow Venus to cool.
  • Venus’ rotation could be sped up and a slight tilt in the axis to match Earth’s rotation and axis.

Numbers 4 and 5 are beyond our current technology, however, solving the 1 through 3 issues are a matter of finding or creating an organism that could float in venus’ upper atmosphere and convert CO₂ to O₂. This could help scientists find a way to remove the excess carbon from Earth’s atmosphere and prevent global warming from becoming a runaway greenhouse effect on our planet.

It should be noted that Earth’s temperature is a delicate balance between incoming and outgoing energy. We don’t know at what point a runaway greenhouse effect kicks in and destroys the energy balance that maintains a near constant temperature on Earth; however, there is a point of no return where evaporating water vapor and CO₂ will absorb more energy from the Sun than what is radiated back into space. If we reach that point, Earth will become another Venus and the human race will cease to exist.

Smoke Adds To Global Warming

18 Thursday Sep 2014

Posted by Paul Kiser in About Reno, Ethics, Green, Health, Politics, Science, solar, Universities

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atmosphere, children, environment, Ethics, Global warming, infrared, King fire, Nevada, Reno, Rim fire, smoke, solar, Sun

Morning smoke haze over Reno, Nevada caused by California King fire

September morning smoke haze over Reno, Nevada caused by California King fire

Seventy-eight percent of the Earth’s atmosphere is nitrogen, and twenty-one percent is oxygen. Both of these gases do not absorb infrared radiation. The heat from the Sun passes through nitrogen and oxygen. When scientists refer to global warming they are not talking about the two gases that make up 99% of our atmosphere.

Global warming is what happens in one percent of the atmosphere. Carbon, water vapor, and other trace gases/particles absorb infrared radiation from the Sun, and from solar infrared radiation that.is reflected off the Earth’s surface. One percent of our air holds the balance between continuity of our climate and rapid variances.

Some are proud of their role in causing devastating environmental change.

Some are proud of their role in causing devastating environmental change.

This summer one of my friends, Dr. Narayan Adhikari, completed his doctoral theses. He studied the rate of infrared absorption in the atmosphere by using instruments that regularly measured the air over various locations in northern Nevada. His research included two significant events that impacted the air quality in the Reno, Nevada area. One event was a dust storm in June of last year and the other was smoke from the Rim fire in California in August of 2013.

Both of these events gave him the opportunity to measure the impact of infrared absorption when the atmosphere has a dramatic increase in amount of aerosol particulates. The results of his studies indicate a significant increase in heating of the atmosphere by infrared absorption during such events. 

This debunks the idea that clouds, smoke, and other ‘sun-blocking’ events might help cool the atmosphere. Smoke from fires, such as the King fire currently burning in California will trap more heat and cause increased global warming.

Other Pages of This Blog

  • About Paul Kiser
  • Common Core: Are You a Good Switch or a Bad Switch?
  • Familius Interruptus: Lessons of a DNA Shocker
  • Moffat County, Colorado: The Story of Two Families
  • Rules on Comments
  • Six Things The United States Must Do
  • Why We Are Here: A 65-Year Historical Perspective of the United States

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