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Asteroid impact avoidance

Asteroid impact avoidance is a astronomy 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 Asteroid impact avoidance rather than just read about it. In short: Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted, preventing destructive impact events. An impact by a sufficiently large asteroid or other NEOs would cause, depending on its impact location, massive tsunamis or multiple firestorms, and an impact winter caused by the sunlight-blocking effect of large quantities of pulveri…

Asteroid impact avoidance — main illustration
Asteroid impact avoidance — illustration

Key takeaways

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

Reference excerpt

Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted, preventing destructive impact events. An impact by a sufficiently large asteroid or other NEOs would cause, depending on its impact location, massive tsunamis or multiple firestorms, and an impact winter caused by the sunlight-blocking effect of large quantities of pulverized rock dust and other debris placed into the stratosphere. A collision 66 million years ago between the Earth and an object approximately 10 kilometers (6 miles) wide is thought to have produced the Chicxulub crater and triggered the Cretaceous–Paleogene extinction event that the scientific community understands to have caused the extinction of all non-avian dinosaurs. While the chances of a major collision are low in the near term, it is a near-certainty that one will happen eventually unless defensive measures are taken. Astronomical events—such as the Shoemaker-Levy 9 impacts on Jupiter and the 2013 Chelyabinsk meteor, along with the growing number of near-Earth objects discovered and catalogued on the Sentry Risk Table—have drawn renewed attention to such threats. The popularity of the 2021 movie Don't Look Up helped to raise awareness of the possibility of avoiding NEOs. Awareness of the threat has grown rapidly during the past few decades, but much more needs to be accomplished before the human population can feel adequately protected from a potentially catastrophic asteroid impact. In 2016, a NASA scientist warned that the Earth is unprepared for such an event. In April 2018, the B612 Foundation reported "It's 100 percent certain we'll be hit by a devastating asteroid, but we're not 100 percent sure when." Also in 2018, physicist Stephen Hawking, in his final book, Brief Answers to the Big Questions, considered an asteroid collision to be the biggest threat to the planet. Several ways of avoiding an asteroid impact have been described. There are two primary ways: to modify the trajectory of the object so that it does not collide with the Earth, or to modify the object by breaking it up so that the resulting fragments do not collide with the Earth or their smaller size reduces the subsequent hazard posed to the Earth. Nonetheless, in March 2019, scientists reported that asteroids may be much more difficult to destroy than thought earlier. An asteroid may reassemble itself due to gravity after being disrupted. In May 2021, NASA astronomers reported that 5 to 10 years of preparation may be needed to avoid a virtual impactor based on a simulated exercise conducted by the 2021 Planetary Defense Conference. In 2022, NASA spacecraft DART impacted Dimorphos, reducing the minor-planet moon's orbital period by 32 minutes. This mission constitutes the first successful attempt at asteroid deflection. In 2027, China plans to launch a deflection mission to the near-Earth object 2015 XF261, with the impact estimated to occur in April 2029.

Deflection efforts

According to expert testimony in the United States Congress in 2013, NASA would require at least five years of preparation before a mission to intercept an asteroid could be launched. In June 2018, the US National Science and Technology Council warned that the United States was unprepared for an asteroid impact event, and developed and released the "National Near-Earth Object Preparedness Strategy Action Plan" to better prepare. Most deflection efforts for a large object require from a year to decades of warning, allowing time to prepare and carry out a collision-avoidance project, as no known planetary defense hardware has yet been developed. It has been estimated that a velocity change of just .035 m/s ÷ t (where t is the number of years until potential impact) is needed to successfully deflect a body on a direct collision trajectory. Thus for a large number of years before impact, much smaller velocity changes are needed. For example, it was estimated there was a high chance of 99942 Apophis swinging by Earth in 2029 with a 10−4 probability of returning on an impact trajectory in 2035 or 2036. It was then determined that a deflection from this potential return trajectory, several years before the swing-by, could be achieved with a velocity change on the order of 10−6 m/s. NASA's Double Asteroid Redirection Test (DART), the world's first full-scale mission to test technology for defending Earth against potential asteroid or comet hazards, launched on a SpaceX Falcon 9 rocket from Space Launch Complex 4 East at Vandenberg Space Force Base in California. An impact by a 10-kilometer (6 mi) asteroid on the Earth has historically caused an extinction-level event due to catastrophic damage to the biosphere. There is also the threat from comets entering the inner Solar System. The impact speed of a long-period comet would likely be several times greater than that of a near-Earth asteroid, making its impact much more destructive; in addition, the warning time is unlikely to be more than a few months. Impacts from objects as small as 50 meters (160 ft) in diameter, which are far more common, are historically extremely destructive regionally (see Barringer crater). Finding out the material composition of the object is also helpful before deciding which strategy is appropriate. Missions like the 2005 Deep Impact probe and the Rosetta spacecraft, have provided valuable information on what to expect. In October 2022, a method of mapping the insides of a potentially problematic asteroid in order to determine the best area for impact was proposed.

… excerpt ends here. Continue reading the full article.

Illustrations

Asteroid impact avoidance: Kinetic impactors such as the one used by the Double Asteroid Redirection Test – its impact with the asteroid moon Dimorphos photographed above – are one of many methods, designed to alter the trajectory of an asteroid to prevent its potential collision with Earth.
Kinetic impactors such as the one used by the Double Asteroid Redirection Test – its impact with the asteroid moon Dimorphos photographed above – are one of many methods, designed to alter the trajectory of an asteroid to prevent its potential collision with Earth.
Asteroid impact avoidance: Damage caused by the Tunguska event. The object was 50–80 meters (160–260 ft) across and exploded 6–10 km (3.7–6.2 mi) above the surface; its explosion flattened 30 million trees and shattered windows hundreds of kilometers away.
Damage caused by the Tunguska event. The object was 50–80 meters (160–260 ft) across and exploded 6–10 km (3.7–6.2 mi) above the surface; its explosion flattened 30 million trees and shattered windows hundreds of kilometers away.
Asteroid impact avoidance: Known Near-Earth objects – as of January 2018Video (0:55; July 23, 2018)(Earth's orbit in white)
Known Near-Earth objects – as of January 2018Video (0:55; July 23, 2018)(Earth's orbit in white)
Asteroid impact avoidance: Frequency of small asteroids roughly 1 to 20 meters in diameter impacting Earth's atmosphere.
Frequency of small asteroids roughly 1 to 20 meters in diameter impacting Earth's atmosphere.
Asteroid impact avoidance: Number of NEOs detected by various projects.
Number of NEOs detected by various projects.

Worked examples

Example 1 — a first encounter with Asteroid impact avoidance

Start with the simplest possible case. Write down what Asteroid impact avoidance claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, 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 Asteroid impact avoidance 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 Asteroid impact avoidance 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 Asteroid impact avoidance

In research
Asteroid impact avoidance appears in astronomy 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 Asteroid impact avoidance 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
Asteroid impact avoidance is common in secondary-school and first-year university syllabi. It links to neighbouring topics Asteroids, Earth, Future problems, so understanding it makes those chapters shorter.
In everyday life
Look for Asteroid impact avoidance 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 Asteroid impact avoidance in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Asteroid impact avoidance 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 Asteroid impact avoidance out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Asteroid impact avoidance in simple terms?

Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted, preventing destructive impact events. An impact by a sufficiently large asteroid or other NEOs would cause, depending on its impact location, massive tsu…

Why does Asteroid impact avoidance matter?

Because it connects several astronomy 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 Asteroid impact avoidance?

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 Asteroid impact avoidance.

Tags

  • Asteroids
  • Earth
  • Future problems
  • Impact events
  • Planetary defense
  • Prevention
  • Space weapons

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