An impact winter is a period of prolonged cold weather due to the impact of a large asteroid or comet on the Earth's surface. If an asteroid were to strike land or a shallow body of water, it would eject an enormous amount of dust, ash, and other material into the atmosphere, blocking the radiation from the sun. This would cause the global temperature to decrease drastically. If an asteroid or comet with the diameter of about 5 km (3.1 mi) or more were to hit in a large deep body of water or explode before hitting the surface, there would still be an enormous amount of debris ejected into the atmosphere. It has been proposed that an impact winter could lead to mass extinction, wiping out many of the world's existing species.
Possibility of impact
Each year, the Earth is hit by 5 m (16 ft) meteoroids that deliver an explosion 50 km (31 mi) above the surface with the power equivalent of one kiloton TNT. The Earth is hit every day by a meteor less than by 5 m (16 ft) in diameter, that disintegrates before reaching the surface. The meteors that do make it to the surface tend to strike unpopulated areas, and cause no harm. A human is more likely to die in a fire, flood, or other natural disaster than to die because of an asteroid or comet impact, which is between a 1 in 3,000 and 1 in 250,000 chance. Another study in 1994 found a 1 in 10,000 chance that the Earth will be hit by a large asteroid or comet with a diameter of about 2 km (1.2 mi) during the next century. This object would be capable of disrupting the ecosphere and would kill a large fraction of the world's population. One such object, Asteroid 1950 DA, currently has a 0.005% chance of colliding with Earth in the year 2880, though when first discovered the probability was 0.3%. The probability goes down as orbits are refined with additional measurements.
In addition there are over 300 short period comets which pass near larger planets, such as Saturn and Jupiter, which can change the trajectory and could potentially put them into an Earth crossing orbit. This could happen for long period comets also but the chance is highest for short period comets. The chance of these directly impacting Earth is far lower than an NEO impact. Victor Clube and Bill Napier support a controversial theory that a short period comet in an Earth crossing orbit doesn't need to impact to be hazardous, as it could disintegrate and cause a dust veil with possibilities of a "nuclear winter" scenario with long term global cooling lasting for thousands of years (which they consider to be similar in probability to a 1 km impact).
Necessary impact factors
The Earth experiences a never ending barrage of cosmic debris. Small particles burn up as they enter the atmosphere and are visible as meteors. Many of them go unnoticed by the average person even though not all of them burn up before they hit the Earth's surface. Those that strike the surface are known as meteorites. So clearly not every object that hits the Earth will cause an extinction level event or even cause any real harm. Objects release most of their kinetic energy in the atmosphere and will explode if they experience a column of atmosphere greater than or equal to their mass. Extinction sized impacts on the Earth occur about every 100 million years. Although extinction events happen very rarely, large projectiles can do severe damage. This section will discuss the nature of the hazards posed by projectiles as a function of their size and composition.
A large asteroid or comet could collide with the Earth's surface with the force of hundreds to thousands of times the force of all the nuclear bombs on the Earth. For example, the K/T boundary impact has been proposed to have caused extinction of all non-avian dinosaurs 66 million years ago. Early estimates of this asteroid's size put it at about 10 km (6.2 mi) in diameter. This means it hit with nearly a force of 1,000,000,000 Mt. That is over five billion times larger than the nuclear bomb yield (16 kilotons) that was dropped on Hiroshima during WW2. This impactor excavated the Chicxulub crater that is 180 km (110 mi) in diameter. With an object this size, dust and debris would still be ejected into the atmosphere even if it hit the ocean, which is only 4 km (2.5 mi) deep. An asteroid, meteor, or comet would remain intact through the atmosphere by virtue of its sheer mass. However, an object smaller than 3 km (1.9 mi) would have to have a strong iron composition to breach the lower atmosphere.
There are three different composition types for an asteroid or comet: metallic, stony, and icy. The composition of the object determines whether or not it will make it to the Earth's surface in one piece, disintegrate before breaching the atmosphere, or break up and explode just before reaching the surface. A metallic object tends to be made up of iron and nickel alloys. These metallic objects are the most likely to impact the surface because they stand up better to the stresses of ram pressure induced flattening and fragmentation during deceleration in the atmosphere. The stony objects, like chondritic meteorites, tend to burn, break up, or explode before leaving the upper atmosphere. Those that do make it to the surface need a minimum energy of about 10 MT or about 50 m (160 ft) diameter to breach the lower atmosphere (this is for a stony object hitting at 20 km/s). The porous cometary-like objects are made up of low-density silicates, organics, ice, and volatile, and often burn up in the upper atmosphere because of their low bulk density (≤1 g/cm3).
Although the asteroids and comets that impact the Earth hit with many times the explosive force of a volcano, the mechanisms of an impact winter are similar to those that occur after a mega-volcanic eruption induced volcanic winter. In this scenario massive amounts of debris is injected into the atmosphere that block out some of the sun's radiation for an extended amount of time, which in turn lowers the mean global temperature up to about 20 K (20 °C) after a year. The two main mechanisms that could lead to an impact winter are mass ejection of regolith and multiple firestorms.
Mass ejection of regolith
In a study conducted by Curt Covey et al., it was found that an asteroid about 10 km (6.2 mi) in diameter with the explosive force of about 108 MT could send upward of about 2.5x1015 kg of 1 µm (1 micrometer) sized aerosol particles into the atmosphere. Anything larger would fall quickly back to the surface. These particles would then be spread throughout the atmosphere and absorb or refract the sunlight before it is able to reach the surface, cooling the planet in a similar fashion as the sulfurous aerosol rising from a megavolcano, producing deep global dimming. This is controversially purported to have occurred following the Toba eruption.
These pulverized rock particles would remain in the atmosphere until dry deposition, and due to their size, they would also act as cloud condensation nuclei and would be washed out by wet deposition/precipitation, but even then, about 15% of the sun's radiation might not reach the surface.[why?] After the first 20 days, the land temperature might drop quickly, by about 13 Kelvin. After about a year, the temperature could rebound by about 6 K, but by this time about one-third of the Northern Hemisphere might be covered in ice.
However, this effect could be largely mitigated, even reversed, by a release of enormous quantities of water vapor and carbon dioxide caused by the initial global heat pulse after the impact. If the asteroid hit an ocean (which would be the case with the majority of impact events), water vapour would form the majority of any ejected matter, and would likely result in a major greenhouse effect and a net increase in temperature.
If the impact event is sufficiently energetic it can cause mantle plume (volcanism) at the antipodal point(the opposite side of the world). This volcanism could alone therefore create a volcanic winter, irrespective of the other impact effects.
In combination with the initial debris ejected into the atmosphere, if the impactor is extremely large (3 km (1.9 mi) or more), like the K/T boundary impactor (estimated 10 km (6.2 mi)), there might be the ignition of multiple fire storms, possibly with a global reach into every dense, and therefore firestorm prone, forest. These wood fires might release enough amounts of water vapor, ash, soot, tar and carbon dioxide into the atmosphere to perturb the climate on their own, and cause the pulverized rock dust cloud blocking the sun to last longer. Alternatively it could cause it to last much shorter, as there would be more water vapor for the rocky aerosol particles to form cloud condensation nuclei. If it causes the dust cloud to last longer, it would prolong the Earth's cooling time, possibly causing thicker ice sheets to form.
Impact on humans
An impact winter would have a devastating effect on humans, as well as the other species on Earth. With the sun's radiation being severely diminished the first thing to go would be plants and animals who survive through the process of photosynthesis. This lack of food would ultimately lead to other mass extinctions of other animals that are higher up on the food chain, and possibly cause up to 25% of the human population to perish. Depending on location and size of the initial impact, the cost of clean-up efforts could be so high as to cause an economic crisis for the survivors. These factors would make life on Earth, for humans, extremely difficult.
With the Earth's atmosphere full of dust and other material, radiation from the sun would be refracted and scattered back into space, and absorbed by this debris. The first effect on the Earth, after the blast wave and potential multiple fire storms, would be the death of most, if not all, of the photosynthetic life forms on Earth. Those in the ocean that survive would possibly become dormant until the sun came out again. Those on land could possibly be kept alive in underground microclimates, with one such example being the Zbrašov aragonite caves, greenhouses in such underground complexes with fossil or nuclear energy power stations could keep artificial sunlight growing lamps on until the atmosphere began to clear. Those outside that were not killed by the lack of sunlight would most likely be killed or kept dormant by the extreme cold of the impact winter. This death of plants might lead to a long period of famine if enough people survived the initial blast wave and would result in increased food costs in undeveloped countries only a few months after the first crop failures. Developed countries wouldn't encounter famine unless the cooling event was to last longer than a year, due to larger canned food and grain stockpiles in these countries. However, if the impactor was similar in size to the K/T boundary impactor, agricultural losses might not be compensated with imports to the northern hemisphere from the southern hemisphere or vice versa. The only way to keep from starving would be for each country to amass at least a year's worth of food for their people. Not many countries have this; the world's average cereal stock levels are only about 30% of the yearly production.
The cost to clean up after an asteroid or comet impact would cost billions to trillions of dollars, depending on the location impacted. An impact in New York City (the 16th most populated city in the world) could cost billions of dollars in financial losses, and it could take years for the financial sector (i.e. stock market) to recover. However, the probability of such a naturally specifically aimed impact would be exceedingly low.
As of 2003 there were about 2300 Near-Earth objects known; 650 of those were larger than 1 km (0.62 mi) in diameter. More than one new one is discovered each year. 500 potentially hazardous objects are known, they are larger than 150 m (490 ft), and may approach the Earth closer than 20 times the distance to the Moon. By the end of the decade we expect to know the orbits of 90% of the kilometer size near-Earth objects.
- Asteroid deflection strategies
- Earth Impact Database
- Impact Event
- List of notable asteroids
- Near Earth Asteroids
- Near-Earth objects
- Nuclear winter
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