Space sunshade

Last updated

A space sunshade or sunshield is a parasol that diverts or otherwise reduces some of the Sun's radiation, preventing it from hitting a spacecraft or planet and thereby reducing its insolation, which results in reduced heating. Light can be diverted by different methods. The concept of the construction of sunshade as a method of climate engineering dates back to the years 1923, 1929, 1957 and 1978 by the physicist Hermann Oberth. [1] [2] [3] [4] Space mirrors in orbit around the Earth with a diameter of 100 to 300 km, as designed by Hermann Oberth, are intended to focus sunlight on individual regions of the Earth’s surface or deflect it into space so that the solar radiation is weakened in a specifically controlled manner for individual regions on the Earth’s surface. First proposed in 1989, another space sunshade concept involves putting a large occulting disc, or technology of equivalent purpose, between the Earth and Sun.

Contents

A sunshade is of particular interest as a climate engineering method for mitigating global warming through solar radiation management. Heightened interest in such projects reflects the concern that internationally negotiated reductions in carbon emissions may be insufficient to stem climate change. [5] [6] Sunshades could also be used to produce space solar power, acting as solar power satellites. Proposed shade designs include a single-piece shade and a shade made by a great number of small objects. Most such proposals contemplate a blocking element at the Sun-Earth L1 Lagrangian point.

Modern proposals are based on some form of distributed sunshade composed of lightweight transparent elements or inflatable "space bubbles" manufactured in space to reduce the cost of launching massive objects to space. [7] [8]

Designs for planetary sunshade

Cloud of small spacecraft

One proposed sunshade would be composed of 16 trillion small disks at the Sun-Earth L1 Lagrangian point, 1.5 million kilometers from Earth and between it and the Sun. Each disk is proposed to have a 0.6-meter diameter and a thickness of about 5 micrometers. The mass of each disk would be about a gram, adding up to a total of almost 20 million tonnes. [9] Such a group of small sunshades that blocks 2% of the sunlight, deflecting it off into space, would be enough to halt global warming. [10] If 100 tonnes of disks were launched to low Earth orbit every day, it would take 550 years to launch all of them.

The individual autonomous flyers building up the cloud of sunshades are proposed not to reflect the sunlight but rather to be transparent lenses, deflecting the light slightly so it does not hit Earth. This minimizes the effect of solar radiation pressure on the units, requiring less effort to hold them in place at the L1 point. An optical prototype has been constructed by Roger Angel with funding from NIAC. [11]

The remaining solar pressure and the fact that the L1 point is one of unstable equilibrium, easily disturbed by the wobble of the Earth due to gravitational effects from the Moon, requires the small autonomous flyers to be capable of maneuvering themselves to hold position. A suggested solution is to place mirrors capable of rotation on the surface of the flyers. By using the solar radiation pressure on the mirrors as solar sails and tilting them in the right direction, the flyer will be capable of altering its speed and direction to keep in position. [12]

Such a group of sunshades would need to occupy an area of about 3.8 million square kilometers if placed at the L1 point [12] (see other lower disc size estimates below).

It would still take years to launch enough of the disks into orbit to have any effect. This means a long lead time. Roger Angel of the University of Arizona [9] presented the idea for a sunshade at the U.S. National Academy of Sciences in April 2006 and won a NASA Institute for Advanced Concepts grant for further research in July 2006. Creating this sunshade in space was estimated to cost in excess of US$130 billion over 20 years with an estimated lifetime of 50-100 years. [13] Thus leading Professor Angel to conclude that "the sunshade is no substitute for developing renewable energy, the only permanent solution. A similar massive level of technological innovation and financial investment could ensure that. But if the planet gets into an abrupt climate crisis that can only be fixed by cooling, it would be good to be ready with some shading solutions that have been worked out." [12] [14]

Lightweight solutions and "Space bubbles"

A more recent design has been proposed by Olivia Borgue and Andreas M. Hein in 2022, proposing a distributed sunshade with a mass on the order of 100,000 tons, composed of ultra-thin polymeric films and SiO2 nanotubes. [7] The author estimated that launching such mass would require 399 yearly launches of a vehicle such as SpaceX Starship for 10 years. [7]

A 2022 concept by MIT Senseable City Lab proposes using thin-film structures ("space bubbles") manufactured in outer space to solve the problem of launching the required mass to space. [15] MIT scientists led by Carlo Ratti believe deflecting 1.8 percent of solar radiation can fully reverse climate change. The full raft of inflatable bubbles would be roughly the size of Brazil and include a control system to regulate its distance from the Sun and optimise its effects. [16] The shell of the thin-film bubbles would be made of silicon, tested in outer space-like conditions at a pressure of .0028 atm and at -50 degrees Celsius. [16] They plan to investigate low vapor-pressure materials to rapidly inflate the bubbles, such as a silicon-based melt or a graphene-reinforced ionic liquid. [16]

One Fresnel lens

The basic function of a space lens to mitigate global warming. A 1,000-kilometre diameter lens is sufficient, and much smaller than what is shown in this simplified image. As a Fresnel lens it would be only a few millimeters thick. Space lens.png
The basic function of a space lens to mitigate global warming. A 1,000-kilometre diameter lens is sufficient, and much smaller than what is shown in this simplified image. As a Fresnel lens it would be only a few millimeters thick.

Several authors have proposed dispersing light before it reaches the Earth by putting a very large lens in space, perhaps at the L1 point between the Earth and the Sun. This plan was proposed in 1989 by J. T. Early. [17] His design involved making a large glass (2,000 km) occulter from lunar material and placing at the L1 point. Issues included the large amount of material needed to make the disc and also the energy to launch it to its orbit. [6]

In 2004, physicist and science fiction author Gregory Benford calculated that a concave rotating Fresnel lens 1000 kilometres across, yet only a few millimeters thick, floating in space at the L1 point, would reduce the solar energy reaching the Earth by approximately 0.5% to 1%. [18]

The cost of such a lens has been disputed. At a science fiction convention in 2004, Benford estimated that it would cost about US$10 billion up front, and another $10 billion in supportive cost during its lifespan. [18]

One diffraction grating

A similar approach involves placing a very large diffraction grating (thin wire mesh) in space, perhaps at the L1 point between the Earth and the Sun. A proposal for a 3,000 ton diffraction mesh was made in 1997 by Edward Teller, Lowell Wood, and Roderick Hyde, [19] although in 2002 these same authors argued for blocking solar radiation in the stratosphere rather than in orbit given then-current space launch technologies. [20]

Other Lower Disc Size Estimates

Recent work by Feinberg (2022) [21] illustrate that lower disc area sizes (factor of approximately 3.5 reduction) are feasible when the background climate response is considered. For example, the background Earth climate would yield less re-radiation and feedback. In addition, disc area sizes can be further reduced by 50 times using an Annual Solar Geoengineering approach as indicated by Feinberg (2024) [22] .

Spacecraft sunshades

The James Webb Space Telescope (JWST) infrared telescope has a layered sunshade to keep the telescope cold.

For spacecraft approaching the Sun, the sunshade is usually called a heatshield. Notable spacecraft [designs] with heatshields include:

See also

Related Research Articles

<span class="mw-page-title-main">Interplanetary spaceflight</span> Crewed or uncrewed travel between stars or planets

Interplanetary spaceflight or interplanetary travel is the crewed or uncrewed travel between stars and planets, usually within a single planetary system. In practice, spaceflights of this type are confined to travel between the planets of the Solar System. Uncrewed space probes have flown to all the observed planets in the Solar System as well as to dwarf planets Pluto and Ceres, and several asteroids. Orbiters and landers return more information than fly-by missions. Crewed flights have landed on the Moon and have been planned, from time to time, for Mars, Venus and Mercury. While many scientists appreciate the knowledge value that uncrewed flights provide, the value of crewed missions is more controversial. Science fiction writers propose a number of benefits, including the mining of asteroids, access to solar power, and room for colonization in the event of an Earth catastrophe.

<span class="mw-page-title-main">Lagrange point</span> Equilibrium points near two orbiting bodies

In celestial mechanics, the Lagrange points are points of equilibrium for small-mass objects under the gravitational influence of two massive orbiting bodies. Mathematically, this involves the solution of the restricted three-body problem.

A statite is a hypothetical type of artificial satellite that employs a solar sail to continuously modify its orbit in ways that gravity alone would not allow. Typically, a statite would use the solar sail to "hover" in a location that would not otherwise be available as a stable geosynchronous orbit. Statites have been proposed that would remain in fixed locations high over Earth's poles, using reflected sunlight to counteract the gravity pulling them down. Statites might also employ their sails to change the shape or velocity of more conventional orbits, depending upon the purpose of the particular statite.

<span class="mw-page-title-main">Solar sail</span> Space propulsion method using Sun radiation

Solar sails are a method of spacecraft propulsion using radiation pressure exerted by sunlight on large surfaces. A number of spaceflight missions to test solar propulsion and navigation have been proposed since the 1980s. The first spacecraft to make use of the technology was IKAROS, launched in 2010.

<span class="mw-page-title-main">Space weather</span> Branch of space physics and aeronomy

Space weather is a branch of space physics and aeronomy, or heliophysics, concerned with the varying conditions within the Solar System and its heliosphere. This includes the effects of the solar wind, especially on the Earth's magnetosphere, ionosphere, thermosphere, and exosphere. Though physically distinct, space weather is analogous to the terrestrial weather of Earth's atmosphere. The term "space weather" was first used in the 1950s and popularized in the 1990s. Later, it prompted research into "space climate", the large-scale and long-term patterns of space weather.

<span class="mw-page-title-main">Solar and Heliospheric Observatory</span> European space observatory

The Solar and Heliospheric Observatory (SOHO) is a European Space Agency (ESA) spacecraft built by a European industrial consortium led by Matra Marconi Space that was launched on a Lockheed Martin Atlas IIAS launch vehicle on 2 December 1995, to study the Sun. It has also discovered over 4,000 comets. It began normal operations in May 1996. It is a joint project between the European Space Agency (ESA) and NASA. SOHO was part of the International Solar Terrestrial Physics Program (ISTP). Originally planned as a two-year mission, SOHO continues to operate after over 25 years in space; the mission has been extended until the end of 2025, subject to review and confirmation by ESA's Science Programme Committee.

<span class="mw-page-title-main">Mars 96</span> Failed Mars mission

Mars 96 was a failed Mars mission launched in 1996 to investigate Mars by the Russian Space Forces and not directly related to the Soviet Mars probe program of the same name. After failure of the second fourth-stage burn, the probe assembly re-entered the Earth's atmosphere, breaking up over a 320 km (200 mi) long portion of the Pacific Ocean, Chile, and Bolivia. The Mars 96 spacecraft was based on the Phobos probes launched to Mars in 1988. They were of a new design at the time and both ultimately failed. For the Mars 96 mission the designers believed they had corrected the flaws of the Phobos probes, but the value of their improvements was never demonstrated due to the destruction of the probe during the launch phase.

<span class="mw-page-title-main">Deep Space Climate Observatory</span> American solar research spacecraft

Deep Space Climate Observatory is a National Oceanic and Atmospheric Administration (NOAA) space weather, space climate, and Earth observation satellite. It was launched by SpaceX on a Falcon 9 v1.1 launch vehicle on 11 February 2015, from Cape Canaveral. This is NOAA's first operational deep space satellite and became its primary system of warning Earth in the event of solar magnetic storms.

In astrodynamics, orbital station-keeping is keeping a spacecraft at a fixed distance from another spacecraft or celestial body. It requires a series of orbital maneuvers made with thruster burns to keep the active craft in the same orbit as its target. For many low Earth orbit satellites, the effects of non-Keplerian forces, i.e. the deviations of the gravitational force of the Earth from that of a homogeneous sphere, gravitational forces from Sun/Moon, solar radiation pressure and air drag, must be counteracted.

Planetary engineering is the development and application of technology for the purpose of influencing the environment of a planet. Planetary engineering encompasses a variety of methods such as terraforming, seeding, and geoengineering.

Climate engineering is a term used for both carbon dioxide removal and solar radiation management, also called solar geoengineering, when applied at a planetary scale. However, they have very different geophysical characteristics which is why the Intergovernmental Panel on Climate Change no longer uses this overarching term. Carbon dioxide removal approaches are part of climate change mitigation. Solar geoengineering involves reflecting some sunlight back to space. All forms of geoengineering are not a standalone solution to climate change, but need to be coupled with other forms of climate change mitigation. Another approach to geoengineering is to increase the Earth's thermal emittance through passive radiative cooling.

<span class="mw-page-title-main">Solar Orbiter</span> European space-based solar observatory

The Solar Orbiter (SolO) is a Sun-observing probe developed by the European Space Agency (ESA) with a National Aeronautics and Space Administration (NASA) contribution. Solar Orbiter, designed to obtain detailed measurements of the inner heliosphere and the nascent solar wind, will also perform close observations of the polar regions of the Sun which is difficult to do from Earth. These observations are important in investigating how the Sun creates and controls its heliosphere.

<span class="mw-page-title-main">Terraforming of Venus</span> Engineering the global environment of Venus to make it suitable for humans

The terraforming of Venus or the terraformation of Venus is the hypothetical process of engineering the global environment of the planet Venus in order to make it suitable for human habitation. Adjustments to the existing environment of Venus to support human life would require at least three major changes to the planet's atmosphere:

  1. Reducing Venus's surface temperature of 737 K
  2. Eliminating most of the planet's dense 9.2 MPa (91 atm) carbon dioxide and sulfur dioxide atmosphere via removal or conversion to some other form
  3. The addition of breathable oxygen to the atmosphere.
<span class="mw-page-title-main">Halo orbit</span> Periodic, three-dimensional orbit

A halo orbit is a periodic, three-dimensional orbit associated with one of the L1, L2 or L3 Lagrange points in the three-body problem of orbital mechanics. Although a Lagrange point is just a point in empty space, its peculiar characteristic is that it can be orbited by a Lissajous orbit or by a halo orbit. These can be thought of as resulting from an interaction between the gravitational pull of the two planetary bodies and the Coriolis and centrifugal force on a spacecraft. Halo orbits exist in any three-body system, e.g., a Sun–Earth–orbiting satellite system or an Earth–Moon–orbiting satellite system. Continuous "families" of both northern and southern halo orbits exist at each Lagrange point. Because halo orbits tend to be unstable, station-keeping using thrusters may be required to keep a satellite on the orbit.

This is a list of climate change topics.

Project Earth is a 2008 reality TV series, hosted by Kevin O'Leary, Jennifer L. Languell, and Mocean Melvin, on the Discovery Channel in which several groups of scientists experiment with radical ideas to slow and/or stop global warming using geoengineering methods.

<span class="mw-page-title-main">Aditya-L1</span> Indias first solar observation mission

Aditya-L1 (/aːd̪it̪jə/) is a coronagraphy spacecraft for studying the solar atmosphere, designed and developed by the Indian Space Research Organisation (ISRO) and various other Indian Space Research Institutes. It is orbiting at about 1.5 million km from Earth in a halo orbit around the Lagrange point 1 (L1) between the Earth and the Sun, where it will study the solar atmosphere, solar magnetic storms, and their impact on the environment around the Earth.

<span class="mw-page-title-main">Solar radiation modification</span> Reflection of sunlight to reduce global warming

Solar radiation modification (SRM), or solar geoengineering, is a type of climate engineering in which sunlight would be reflected back to outer space to limit or offset human-caused climate change. There are multiple potential approaches, with stratospheric aerosol injection being the most-studied, followed by marine cloud brightening (MCB). SRM is not a substitute for reducing greenhouse gas emissions but could be a temporary measure to limit climate-change impacts while emissions are reduced and carbon dioxide is removed.

<span class="mw-page-title-main">Space mirror (climate engineering)</span> Artificial satellites designed to change the amount of solar radiation that impacts Earth

Space mirrors are satellites that are designed to change the amount of solar radiation that impacts the Earth as a form of climate engineering. 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. They have been theorised as a method of solar geoengineering by creating a space sunshade to deflect sunlight and counter global warming.

References

  1. Oberth, Hermann (1984) [1923]. Die Rakete zu den Planetenräumen (in German). Michaels-Verlag Germany. pp. 87–88.
  2. Oberth, Hermann (1970) [1929]. ways to spaceflight. NASA. pp. 481–506. Retrieved 21 December 2017 via archiv.org.
  3. Oberth, Hermann (1957). Menschen im Weltraum (in German). Econ Duesseldorf Germany. pp. 125–182.
  4. Oberth, Hermann (1978). Der Weltraumspiegel (in German). Kriterion Bucharest.
  5. Hickman, John (2018). "The Political Economy of a Planetary Sunshade". Astropolitics. 16 (1): 49–58. Bibcode:2018AstPo..16...49H. doi:10.1080/14777622.2018.1436360. S2CID   148608737.
  6. 1 2 Gorvett, Zaria (26 April 2016). "How a giant space umbrella could stop global warming". BBC. Archived from the original on 20 December 2016. Retrieved 7 December 2016.
  7. 1 2 3 Borgue, Olivia; Hein, Andreas M. (2022). "Transparent occulters: A nearly zero-radiation pressure sunshade to support climate change mitigation". Acta Astronautica. 203 (in press): 308–318. doi: 10.1016/j.actaastro.2022.12.006 . S2CID   254479656.
  8. "Space Bubbles Could Be the Wild Idea We Need to Deflect Solar Radiation". Popular Mechanics. 7 July 2022. Retrieved 23 May 2023.
  9. 1 2 "Space sunshade might be feasible in global warming emergency". EurekAlert. 3 November 2006. Archived from the original on 23 October 2020. Retrieved 11 November 2010.
  10. "Global Sunshade". BBC News. 19 February 2007. Archived from the original on 1 March 2007. Retrieved 11 November 2010.
  11. Tnenbaum, David (23 April 2007). "Pies in the Sky: A Solution to Global Warming". Astrobiology Magazine. Archived from the original on 2 February 2016. Retrieved 14 November 2010.
  12. 1 2 3 Angel, Roger (18 September 2006). "Feasibility of cooling the Earth with a cloud of small spacecraft near the inner Lagrange point (L1)". Proceedings of the National Academy of Sciences of the United States of America. PNAS. 103 (46): 17184–9. Bibcode:2006PNAS..10317184A. doi: 10.1073/pnas.0608163103 . PMC   1859907 . PMID   17085589.
  13. Konecny, Pavel (6 December 2018). "We need SpaceX BFR not just get us to MARS but to save EARTH from Global Warming". Medium. Archived from the original on 22 November 2021. Retrieved 11 March 2019.
  14. "Space Sunshade Might Be Feasible In Global Warming Emergency" (Press release). University of Arizona. 6 November 2006. Archived from the original on 16 March 2010. Retrieved 29 April 2009.
  15. "Space bubbles". MIT Senseable City Lab. Retrieved 24 May 2023.
  16. 1 2 3 "Space Bubbles Could Be the Wild Idea We Need to Deflect Solar Radiation". Popular Mechanics. 7 July 2022. Retrieved 23 May 2023.
  17. J. T. Early (1989), "Space-Based Solar Shield To Offset Greenhouse Effect", Journal of the British Interplanetary Society, vol. 42, pp. 567–569, Bibcode:1989JBIS...42..567E . This proposal is also discussed in footnote 23 of Edward Teller; Roderick Hyde & Lowell Wood (1997), Global Warming and Ice Ages: Prospects for Physics-Based Modulation of Global Change (PDF), Lawrence Livermore National Laboratory, archived (PDF) from the original on 27 January 2016, retrieved 30 October 2010.
  18. 1 2 See Russell Dovey, "Supervillainy: Astroengineering Global Warming Archived 4 August 2012 at archive.today and Bill Christensen, "Reduce Global Warming by Blocking Sunlight" Archived 2009-04-17 at the Wayback Machine .
  19. Edward Teller; Roderick Hyde & Lowell Wood (1997), Global Warming and Ice Ages: Prospects for Physics-Based Modulation of Global Change (PDF), Lawrence Livermore National Laboratory, archived (PDF) from the original on 27 January 2016, retrieved 30 October 2010. See pages 10–14 in particular.
  20. Edward Teller, Roderick Hyde & Lowell Wood (2002), Active Climate Stabilization: Practical Physics-Based Approaches to Prevention of Climate Change (PDF), Lawrence Livermore National Laboratory, archived (PDF) from the original on 13 May 2009, retrieved 30 October 2010
  21. Feinberg, Alec (2022). "Solar Geoengineering Modeling and Applications for Mitigating Global Warming: Assessing Key Parameters and the Urban Heat Island Influence". Frontiers in Climate. 4. doi: 10.3389/fclim.2022.870071 . ISSN   2624-9553.
  22. Feinberg, Alec (February 2024). "Annual Solar Geoengineering: Mitigating Yearly Global Warming Increases". Climate. 12 (2): 26. doi: 10.3390/cli12020026 . ISSN   2225-1154.