*Black hole evaporation time varies with mass. For a black hole with the mass of our Sun (1 solar mass), it would take approximately 10671067 years to evaporate due to Hawking radiation. Larger black holes have even longer evaporation times, making the process exceedingly slow on astronomical timescales.*

## Black Hole Evaporation Time Calculator

Here is a table summarizing the evaporation time of black holes of various masses, assuming Hawking radiation as the mechanism for evaporation. The times are given in years:

Black Hole Mass | Evaporation Time (Years) |
---|---|

1 Solar Mass (M☉) | Approximately 10671067 years |

10 Solar Masses | Approximately 10661066 years |

100 Solar Masses | Approximately 10651065 years |

1,000 Solar Masses | Approximately 10641064 years |

1 Million Solar Masses | Approximately 10591059 years |

1 Billion Solar Masses | Approximately 10541054 years |

1 Trillion Solar Masses | Approximately 10491049 years |

Please note that these timescales are theoretical estimates and are extremely long, especially for larger black holes. The actual rate of black hole evaporation would depend on various factors, including the surrounding environment and any accretion of additional mass.

## FAQs

**Do black holes evaporate over time?** Yes, black holes do evaporate over time due to Hawking radiation, a quantum effect that causes them to lose mass and energy gradually.

**How long would it take to evaporate a black hole the size of the Sun?** It would take an incredibly long time, on the order of 10671067 years, for a black hole with the mass of the Sun to evaporate completely.

**How much is 1 minute in a black hole?** Time near a black hole can be significantly dilated compared to time in a distant observer’s frame. The exact time dilation depends on the black hole’s mass and your proximity to it. Near the event horizon of a massive black hole, one minute for you could correspond to a much longer time for a distant observer, possibly even millions or billions of years.

**How long is 1 hour in a black hole?** Similar to the previous answer, the length of an hour near a black hole would depend on the black hole’s mass and your proximity to it. Near the event horizon of a massive black hole, one hour for you could correspond to an extremely long time for a distant observer.

**Will black holes eventually dissipate?** Yes, black holes will eventually dissipate over an extremely long period of time due to Hawking radiation, which causes them to lose mass and energy. However, this process takes an extraordinarily long time for large black holes, and it’s currently not observable within the age of the universe.

**What happens after the last black hole evaporates?** After the last black hole evaporates, there will be no more black holes in the universe. The remnants of the black holes will have radiated away into particles and energy, contributing to the overall heat and entropy of the universe. At this point, the universe would consist of various particles, radiation, and possibly other exotic forms of matter, with no large-scale gravitational singularities.

**Do black holes stay active forever?** No, black holes do not stay active forever. They gradually lose mass and energy through Hawking radiation and will eventually dissipate completely if they don’t accrete more matter to counteract this process.

**Do black holes eventually implode?** Black holes do not implode in the conventional sense. Instead, they gradually lose mass and energy through Hawking radiation until they reach a point where they no longer have sufficient mass to maintain their event horizon. At this point, they effectively “evaporate” rather than implode.

**Is information lost when a black hole evaporates?** The issue of whether information is lost when a black hole evaporates is known as the black hole information paradox. It is a topic of ongoing debate in theoretical physics. According to classical physics, information that falls into a black hole is seemingly lost forever, violating the principle of information conservation. However, some theories, such as those involving black hole complementarity or firewalls, attempt to reconcile this paradox and preserve information in some way.

**How many suns does it take to fill a black hole?** A black hole’s mass is typically measured in terms of solar masses (M☉), where 1 solar mass is approximately equal to the mass of our Sun (about 2 x 10^30 kilograms). So, to “fill” a black hole with the mass of, for example, 10 solar masses, you would need 10 Suns’ worth of mass.

**How fast would a micro black hole evaporate?** Micro black holes, if they exist, would evaporate very quickly due to Hawking radiation. The evaporation time is inversely proportional to the black hole’s mass, so smaller black holes evaporate faster. Micro black holes would likely evaporate in a fraction of a second or even less.

**How long will it take for the black holes of the universe to evaporate according to the heat death scenario?** The time it would take for all black holes in the universe to evaporate completely is an extraordinarily long period, far longer than the current age of the universe. It’s estimated to take trillions or more years, making it a scenario that goes well beyond the timescale of the heat death of the universe, which is itself a concept that occurs on an even longer timescale.

**What is evaporation rate speed?** The evaporation rate speed is the rate at which a substance undergoes evaporation, typically measured in units like grams per second or moles per second. It depends on factors such as temperature, surface area, and the properties of the substance itself.

**How long is evaporation?** Evaporation is a continuous process, and its duration depends on various factors, including the substance being evaporated, the environmental conditions (e.g., temperature and humidity), and the surface area exposed to the evaporation process. It can range from seconds to hours or longer.

**Does evaporation take time?** Yes, evaporation takes time. It is a gradual process by which a substance transitions from its liquid state to its gaseous state. The exact time it takes for evaporation to occur depends on the factors mentioned earlier.

**How long is 1 day in a black hole?** The length of a day near a black hole would depend on the black hole’s mass and your proximity to it, leading to significant time dilation effects. Near the event horizon of a massive black hole, one day for you could correspond to an extremely long time for a distant observer.

**How fast is a black hole in mph?** Black holes don’t have a “speed” in the traditional sense because they don’t move through space like objects with mass. Instead, they create a gravitational field that warps spacetime around them. Objects that get too close to a black hole may fall into its gravitational pull and ultimately cross its event horizon.

**Is time slower at a black hole?** Yes, time is slower near a black hole due to the gravitational time dilation effect predicted by Einstein’s theory of general relativity. The closer you are to a massive object like a black hole, the slower time appears to pass compared to observers at a greater distance.

**Would you age in a black hole?** You would continue to experience the passage of time inside a black hole, but due to extreme gravitational time dilation, your perception of time would be significantly different from that of observers far away from the black hole. Time dilation effects near a black hole can be so extreme that even a short time for you could correspond to an immense amount of time for distant observers.

**Does time become space in black holes?** Time and space are intimately linked in the fabric of spacetime according to the theory of general relativity. In the vicinity of a black hole, the extreme curvature of spacetime causes time and space to behave in unusual ways, leading to significant time dilation and space compression effects. However, time itself doesn’t “become” space.

**What happens when 2 black holes collide?** When two black holes collide, they merge to form a larger black hole in a process called a black hole merger or coalescence. This event releases a tremendous amount of energy in the form of gravitational waves, which are ripples in spacetime. These gravitational waves carry away energy and angular momentum from the system, causing the two black holes to spiral inward and eventually merge into a single, more massive black hole.

**What can destroy a black hole?** In the context of general relativity and current understanding of physics, black holes are exceptionally stable objects that are difficult to destroy by conventional means. They can lose mass and energy over time due to Hawking radiation, but this is a slow process. In practice, extreme astrophysical events, such as the collision and merger of black holes, can change their properties, but they do not “destroy” black holes in the sense of making them disappear completely.

**Do black holes emit anything?** Yes, black holes emit Hawking radiation, which is a form of thermal radiation consisting of particles, primarily photons and virtual particle-antiparticle pairs, that are created near the event horizon. This radiation causes black holes to gradually lose mass and energy over time.

**What is the last point of a black hole?** The “last point” of a black hole typically refers to its singularity, which is the central point of infinite density within the black hole. This is a theoretical concept where the laws of physics as we know them break down. The singularity is hidden behind the event horizon, making it inaccessible and not directly observable.

**What is the closest black hole to Earth?** The closest known black hole to Earth is likely V616 Monocerotis, also known as A0620-00. It’s located in the constellation Monoceros and is estimated to be about 3,000 light-years away from Earth.

**What is the lifetime of a black hole?** The lifetime of a black hole, in terms of Hawking radiation, depends on its mass. Smaller black holes evaporate more quickly than larger ones. For a black hole with the mass of the Sun, it would take an extremely long time, on the order of 10671067 years, to evaporate completely.

**Can a dormant black hole become active again?** Black holes are not considered “dormant” or “active” in the same way that some astronomical objects like stars or volcanoes are. Once a black hole forms, it remains a black hole. Its behavior is determined by its mass and the surrounding environment, but it doesn’t switch between states of dormancy and activity as other objects might.

**How will the universe end?** The ultimate fate of the universe is a topic of ongoing scientific research and speculation. There are several proposed scenarios, including the Big Freeze (heat death), Big Crunch, and Big Rip. The most widely accepted current model suggests that the universe will continue to expand indefinitely, leading to the eventual cooling and fading of all matter and energy, resulting in the heat death scenario.

**Do we live inside a black hole?** The idea that our universe is inside a black hole is a speculative hypothesis, but it’s not widely accepted in mainstream cosmology. There is no conclusive evidence to support this idea, and it remains a topic of debate among theoretical physicists.

**Could you theoretically destroy a black hole?** In the context of current physics and our understanding of black holes, it’s not clear if it’s theoretically possible to destroy a black hole. Black holes are extremely stable and have immense gravitational forces. Their ultimate fate, as described by Hawking radiation, is a very slow process. To date, there are no known mechanisms or processes that can rapidly and completely destroy a black hole.

**Do black holes create new universes?** The idea that black holes could potentially create new universes is a speculative concept derived from certain interpretations of quantum physics and the multiverse hypothesis. In some theoretical models, black holes might give rise to new universes through processes related to the nature of spacetime and quantum fluctuations. However, this idea is highly speculative and remains a topic of debate and exploration in theoretical physics.

**Are black holes eternal?** Black holes are not eternal in the sense that they eventually lose mass and energy through Hawking radiation and can eventually evaporate completely. However, the timescales involved are so vast that they may persist for an extraordinarily long time.

**What is the black hole paradox?** The black hole information paradox is a long-standing problem in theoretical physics. It arises from the apparent conflict between the principles of quantum mechanics and general relativity in the context of black holes. According to quantum mechanics, information is always conserved, but general relativity suggests that information that falls into a black hole may be lost forever. Resolving this paradox is an ongoing challenge in theoretical physics.

**Has anything ever escaped a black hole?** Based on our current understanding of black holes, nothing can escape from within the event horizon of a black hole. Anything that crosses the event horizon is effectively trapped, and no information or matter from inside the event horizon can be observed by external observers.

**How can a black hole evaporate if nothing can escape it?** The process of black hole evaporation, as described by Stephen Hawking, involves the creation of particle-antiparticle pairs near the event horizon. One particle falls into the black hole, while the other escapes as Hawking radiation. Over time, this process leads to a gradual loss of mass and energy by the black hole, causing it to evaporate.

**What is the largest black hole ever found?** The largest known black hole in terms of mass is TON 618, located in the Ursa Major constellation. It is estimated to have a mass of around 66 billion times that of our Sun.

**How big would a black hole be with the mass of the Sun?** A black hole with the mass of the Sun would have a size determined by its event horizon, which is roughly 2.95 kilometers (about 1.83 miles) in radius.

**What is the biggest black hole in the whole universe?** TON 618, as mentioned earlier, is one of the largest black holes known, but there may be even larger black holes yet to be discovered in the universe.

**How small of a black hole does it take to destroy the Earth?** The size of a black hole that could potentially destroy the Earth would depend on its mass and distance from our planet. However, such an event is highly unlikely, as there are no known black holes in our immediate vicinity that pose a threat to Earth.

**How long is 1 minute near a black hole?** The length of 1 minute near a black hole would depend on the black hole’s mass and your proximity to it, causing significant time dilation effects. Near the event horizon of a massive black hole, 1 minute for you could correspond to an extremely long time for a distant observer.

**What is the temperature inside a black hole?** The concept of temperature inside a black hole is not well-defined in the same way it is for everyday objects. Black holes have a temperature associated with their Hawking radiation, but this temperature is inversely proportional to their mass and is extremely low for macroscopic black holes. For smaller black holes, such as primordial black holes, the temperature can be higher but still very low in absolute terms.

**How long would it take to evaporate a black hole the size of the sun?** As mentioned earlier, it would take an extremely long time, on the order of 10671067 years, for a black hole with the mass of the Sun to evaporate completely through Hawking radiation.

**How long would it take a 1kg black hole to evaporate?** The time it would take for a 1 kg black hole to evaporate through Hawking radiation is on the order of 10241024 years. Such a small black hole would evaporate relatively quickly compared to larger ones.

**Which is the highest rate of evaporation?** The highest rate of evaporation typically occurs under conditions of high temperature, low humidity, and a large surface area. These conditions maximize the rate at which molecules transition from a liquid to a gaseous state. However, the specific rate of evaporation can vary depending on the substance and environmental factors.

**How do you calculate the speed of evaporation?** The speed of evaporation depends on various factors, including temperature, humidity, and the surface area of the substance exposed to the environment. It can be calculated using mathematical models such as the diffusion equation, but the exact calculation can be complex and depends on the specific conditions.

**Does evaporation ever stop?** Evaporation can slow down or even stop when the environmental conditions are no longer conducive to it. For example, when the air becomes saturated with moisture (reaches 100% humidity), further evaporation may cease because there is no more room for additional water vapor in the air.

**At what temperature does evaporation occur fastest?** Evaporation generally occurs fastest at higher temperatures because higher temperatures provide more energy to the molecules in the liquid, allowing them to escape into the gaseous state more readily. However, the rate of evaporation is also influenced by other factors, such as humidity and pressure.

**Why does evaporation take so long?** The time it takes for evaporation to occur depends on several factors, including the substance being evaporated, the environmental conditions, and the surface area exposed to evaporation. While evaporation can be a relatively fast process in certain conditions, it may take longer in situations where these factors are less favorable.

**Does light speed up evaporation?** Light itself does not directly speed up evaporation. However, the presence of light can indirectly influence the rate of evaporation by heating the substance being evaporated. Increased temperature, which can result from exposure to light, can accelerate the rate of evaporation.

**Is evaporation slower or faster?** The rate of evaporation can vary widely depending on the specific conditions. Evaporation tends to be faster at higher temperatures, with low humidity, and when there is a larger surface area exposed to the environment. Conversely, evaporation is slower at lower temperatures, with high humidity, and in the absence of favorable conditions.

**Where is evaporation faster?** Evaporation is generally faster in environments with the following conditions:

- High temperatures
- Low humidity
- A large surface area exposed to the air

**Is time Infinite in a black hole?** Time is not infinite inside a black hole, but the extreme gravitational time dilation near the black hole’s singularity can cause time to appear to pass very slowly or differently compared to observers outside the black hole. However, it does not mean that time is infinite within the black hole.

**How much is 1 minute in a black hole?** The length of 1 minute inside a black hole would depend on the black hole’s mass and your proximity to it, causing significant time dilation effects. Near the event horizon of a massive black hole, 1 minute for you could correspond to an extremely long time for a distant observer.

**Do black holes evaporate?** Yes, black holes do evaporate over time due to Hawking radiation, which causes them to lose mass and energy gradually.

**What is the fastest thing in the universe?** The fastest known phenomenon in the universe is the speed of light in a vacuum, which is approximately 299,792,458 meters per second (about 186,282 miles per second).

**How far back in time is a light year?** A light year is a unit of distance, not time. It represents the distance that light travels in one year. To determine how far back in time you are looking when observing an object one light year away, you are effectively seeing that object as it was one year ago.

**How fast is the speed of light?** The speed of light in a vacuum is approximately 299,792,458 meters per second, which is approximately 186,282 miles per second.

**How slow would you age near a black hole?** Near a black hole, you would age more slowly compared to someone who is farther away from the black hole due to gravitational time dilation. The closer you are to the black hole, the greater the time dilation effect.

**Can we go to past or future in black hole?** According to our current understanding of physics, it is unlikely that black holes can be used as time machines to travel to the past or future. While they can cause significant time dilation effects, they do not provide a means for deliberate time travel. Time dilation effects near a black hole would affect the passage of time for an observer relative to distant observers but would not enable backward time travel. Time travel remains a topic of theoretical exploration in physics, but it is currently speculative and not realized in practice.

GEG Calculators is a comprehensive online platform that offers a wide range of calculators to cater to various needs. With over 300 calculators covering finance, health, science, mathematics, and more, GEG Calculators provides users with accurate and convenient tools for everyday calculations. The website’s user-friendly interface ensures easy navigation and accessibility, making it suitable for people from all walks of life. Whether it’s financial planning, health assessments, or educational purposes, GEG Calculators has a calculator to suit every requirement. With its reliable and up-to-date calculations, GEG Calculators has become a go-to resource for individuals, professionals, and students seeking quick and precise results for their calculations.