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Space mirror

Space mirror is a earth science topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Space mirror rather than just read about it. In short: Solar mirrors in space can be used to change the amount of sunlight that reaches the Earth. The concept was first theorised in 1923 by physicist Hermann Oberth and later developed in the 1980s by other scientists.

Space mirror — main illustration
Space mirror — illustration

Key takeaways

  • Space mirror belongs to earth science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Space mirror to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Space mirror from memory before moving on to harder problems.

Reference excerpt

Solar mirrors in space can be used to change the amount of sunlight that reaches the Earth. The concept was first theorised in 1923 by physicist Hermann Oberth and later developed in the 1980s by other scientists. Space mirrors can be used to increase or decrease the amount of solar energy that reaches a specific point of the earth for various purposes. There have been several proposed implementations of the space mirror concept but none have been implemented thus far other than the Znamya experiment by Russia, due to logistical concerns and challenges of deployment. Znamya successfully tested reflecting more sunlight to Earth.

Oberth's proposal In 1923, Hermann Oberth proposed the construction of space mirrors with a diameter of 100 to 300 km in his book "Die Rakete zu den Planetenräumen". Oberth wrote that a mirror of 100 km diameter "could make broad stretches of land in the north habitable by using diffused light to heat, and in our latitudes it could prevent the feared spring freezes (ice men) in addition to night frosts in the spring and autumn, thereby saving the fruit and vegetable harvests of entire countries." Oberth's 1929 book "Wege zur Raumschiffahrt" (Ways to Spaceflight) expanded on this proposal, giving further details of a reflector constructed of facets of 5 µm thick sodium metal, steerable by electrostatic repulsion. The facets would be held in place by a rotating wire net. He warned of the military applications of such mirrors: "munitions factories can be exploded with it, tornadoes and thunderstorms produced, marching troops and their reserves destroyed, whole cities burned, and generally the greatest of damage done." Oberth estimated that such a reflector would cost only 3 billion Reichsmark and take 15 years to build. Oberth continued to promote his space mirror idea in books published in 1957 and 1978. Since the high cost of spaceflight was by then apparent, Oberth proposed that components should be produced from lunar minerals on the Moon, because its lower gravitational pull requires less energy to launch the components into lunar orbit. In addition, the earth's atmosphere is not burdened by many rocket launches. From the lunar surface, the components would be launched into the lunar orbit by an electromagnetic lunar slingshot and "stacked" at a 60° libration point. From there, the components could be transported into orbit with the electric spaceships he had designed with little recoil, and there they would be assembled into mirrors with a diameter of 100 to 300 km. In 1978 he estimated that the realization could be expected between 2018 and 2038.

Mirror distance and spot size Oberth remarked that "it is impossible to concentrate the light of a 100,000 km-wide reflector on the space of one hectare, as Gail describes it in his novel, The Stone from the Moon". Assuming a small (<10 km) mirror, the spot size is limited by:

d a > D A {\displaystyle {\frac {d}{a}}>{\frac {D}{A}}}

where d is the diameter of the spot of light on the Earth, a is the distance from the mirror to the Earth, D is the diameter of the Sun, and A is the distance from the mirror to the Sun. This is independent of the size or shape of the mirror. For example, a mirror orbiting at 625 km, as proposed by Reflect Orbital, cannot produce a spot smaller than about 2.9 km.

Sunshades

Since 1989, concern about global warming has led scientists to propose various space structures that would reduce the amount of sunlight reaching the Earth, termed geoengineering or solar radiation modification. Some of these proposals use mirrors, either as a solar sail or to provide heat and light as an additional benefit. Lowell Wood, a researcher at the Lawrence Livermore National Laboratory, proposed sending a single, massive mirror into orbit at Lagrange point L1, approximately one million miles away from Earth. The space mirror would be able to remain in orbit without any additional energy supplies and continue to block sunlight. In 2006, Roger Angel, a researcher at the University of Arizona, proposed sending millions of smaller space mirrors as opposed to one large mirror to reduce costs and increase feasibility as a single mirror would need to be approximately 600,000 square miles to block just one percent of sunlight. In 2002, Jerome Pearson at STAR Technology and Research proposed using a network of steerable space mirrors "to form a broad, flat ring like those of Saturn". The proposal, updated in 2006, would require about 5 billion kilograms (1.1×1010 lb) of spacecraft mass costing an estimated $125–500 billion. This would reduce the global temperature by an estimated 1.63K, and would additionally provide controllable evening illumination. Climate experts have cautioned that geoengineering proposals like space mirrors, while potentially being able to cool the planet, would not provide any benefit for other climate related problems like high acidity levels in the ocean due to the build up of carbon. In the past, many scientists have also resisted the idea of using geoengineering to curb climate change, as the risks of causing adverse effects were too great and they worried it would encourage people to continue to use fossil fuels that contribute to that change.

Znamya

The first practical attempt at reflecting sunlight was made in the 1990s by the Russian Federal Space Agency under project Znamya. Intended to provide lighting during Russia's long winter nights, it consisted of three experiments: the Znamya 1, Znamya 2 experiment, and the failed Znamya 2.5. The Znamya 1 was a ground experiment that never was launched. The Znamya 2 was launched into a suborbital trajectory in 1992. It was a 20-metre (66 ft) circular mirror. For several hours, it provided a bright light of a width of 5km and with the luminosity of a full moon. The Znamya 2.5 was a 25-metre (82 ft) mirror which was launched into orbit in 1999 but failed during deployment. Znamya 3 would have been a 60–70 metre mirror, but the project was canceled.

Reflect Orbital

… excerpt ends here. Continue reading the full article.

Illustrations

Space mirror: Znamya-2, which was deployed as part of a series of orbital space mirror experiments in the 1990s by Russia.
Znamya-2, which was deployed as part of a series of orbital space mirror experiments in the 1990s by Russia.

Worked examples

Example 1 — a first encounter with Space mirror

Start with the simplest possible case. Write down what Space mirror claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In earth science, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Space mirror before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Space mirror ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Space mirror

In research
Space mirror appears in earth science research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Space mirror in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Space mirror is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1923 in science, Climate change mitigation, Geoengineering, so understanding it makes those chapters shorter.
In everyday life
Look for Space mirror outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

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How to study Space mirror in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Space mirror means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Space mirror out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Space mirror in simple terms?

Solar mirrors in space can be used to change the amount of sunlight that reaches the Earth. The concept was first theorised in 1923 by physicist Hermann Oberth and later developed in the 1980s by other scientists.

Why does Space mirror matter?

Because it connects several earth science ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Space mirror?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Space mirror.

Tags

  • 1923 in science
  • Climate change mitigation
  • Geoengineering
  • Mirrors
  • Satellites

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