METEORITES FALLS 101
Meteorites are rocks that come from space and land on Earth. They are formed from asteroids, comets, or other space debris that fly around our solar system. When a meteorite falls through the Earth's atmosphere, it heats up and produces a bright streak of light in the sky, which we call a shooting star. If the meteorite is big enough and doesn't completely burn up, it can land on the Earth's surface.
Meteorites come in all shapes and sizes, and they can contain different types of minerals and other materials. Some are very small and only weigh a few grams, while others are huge and weigh thousands of kilograms. Scientists study meteorites to learn more about the history of our solar system, including how the planets formed and what materials were present when the solar system was first created. They can also tell us more about the composition of other celestial bodies in our solar system and beyond. Meteorites are really cool because they are pieces of space that we can actually touch and study up close!
METEORITE COLLECTING
Meteorite collecting is the activity of searching for and collecting rocks that have fallen from space and landed on the Earth's surface. Meteorite hunters use a variety of methods to find these space rocks, including searching in areas where meteorites are known to have fallen in the past, using metal detectors to locate iron-rich meteorites, and analyzing satellite images to identify potential meteorite impact sites.
Once a meteorite has been located, it must be carefully collected and preserved. This involves using specialized tools and techniques to extract the meteorite from the surrounding soil or rocks without damaging it. The meteorite is then cleaned and cataloged, and samples may be taken for scientific analysis.
Meteorite collecting can be a challenging and exciting hobby, as it involves searching for rare and valuable objects that have traveled through space and survived the intense heat and pressure of atmospheric entry. It can also be a way to contribute to scientific research, as many meteorites have important information about the formation and evolution of our solar system.
However, it's important to note that meteorite collecting can also have legal and ethical considerations. Some countries have laws that regulate the collection and sale of meteorites, and some private landowners may not allow people to collect on their property. Additionally, it's important to respect the cultural significance of meteorites to certain indigenous communities, who may view them as sacred objects. As with any hobby or activity, it's important to do your research and follow the appropriate guidelines and best practices.ย
HOW TO FIND METEORITES
This is a step-by-step guide on how to locate meteorite falls using weather radar. The best approach is to have several people using this technique, and then to share their findings to reach a consensus on whether or not they have a searchable event.ย
STEP ONE
Keep an eye out for reports of large, bright events that may indicate a meteorite fall through these resources:
The American Meteor Society : https://www.amsmeteors.com
The Latest Worldwide Meteor/Meteorite News : http://lunarmeteoritehunters.blogspot.com
International Meteor Organization : http://lunarmeteoritehunters.blogspot.com
STEP TWO
Narrow down the search area:
Radar imagery can contain a lot of features, to include weather, birds, bats, aircraft, and "radar noise". The following kinds of data can help narrow down the search area, increasing the likelihood of identifying a meteorite fall if it is visible on radar.
Eyewitnesses
Beyond eyewitness report collections like those in the AMS and IMO websites, interviewing eyewitnesses firsthand can yield useful information. Single EW reports are often contain a measure of error, but accruing many of them may produce a small search area.
Seismic Data
Seismometers are excellent for locating meteorite falls. Fireballs that penetrate deeply enough into the atmosphere to generate sonic booms (and are therefore good candidates to generate meteorite falls) can produce signals in seismometer data if seismometers are nearby.
The consortium group, Incorporated Research Institutions for Seismology (IRIS) maintains an online database of seismometer data from around the world. Calculating a fireball end point from seismometry data is not straightforward, and we suggest teaming up with an expert on the subject. This technique is superb, however, producing fireball terminus locations, altitudes, and timing.
Satellite Imagery
http://www.nhc.noaa.gov/satellite.php
Most civilian imaging satellites are weather satellites, and they only collect images every fifteen minutes or longer. Detecting a fireball would require that the fireball occur just as the satelliteรขโฌโขs camera is taking its image, which is unlikely. In the future it may be possible to obtain real-time imagery but for now this technique is of limited utility.
The GOES Geostationary Lightning Mapper (GLM)
https://www.goes-r.gov/spacesegment/glm.html
This new sensor is found on the NOAA Geostationary Operational Environment Satellite and is very useful for detecting bright fireballs, because this instrument searches for lightning by collecting data on bright flashes on a continuous basis. Because meteors are short-lived, bright flashes like lightning, they show up in the GLM data products. This new sensor is currently in development and constant data feeds are not yet widely available.
Infrasound
Infrasound refers to very low frequency noise, which can travel long distances and is useful for narrowing down the location of an event like a meteorite fall. No public sources of infrasound data are currently available.
STEP THREE
Retrieve and analyze weather radar data to search for signatures of a meteorite fall:
Finding meteorite falls in weather radar imagery requires practice and patience. Fortunately the software and data are freely available. Weather and Climate Toolkit.
NCDC Weather and Climate Toolkit
http://www.ncdc.noaa.gov/wct/tutorials/
Click on the link above to download the Weather and Climate Toolkit radar visualization software provided by the NOAA. Take advantage of the tutorials! Your goal is to learn how to download radar data and search it for meteorite falls.
Features Signifying a Meteorite Fall
Meteorite falls are often (but not always) linear features, with the long axis often aligned in the direction of ambient winds. Meteorite falls appear in radar imagery after the fireball has gone out, and after meteorites have sufficient time to fall from the fireball terminus (roughly 20 km high) down to where the radar can detect them (approximately 10 km and lower altitudes). This normally takes about 2 minutes to occur.
Falling meteorites then appear at or near the site identified by eyewitnesses or the other sources named above. Meteorites are size-sorted in their fall from the fireball terminus, with large meteorites falling fastest and smaller ones requiring a longer time to reach the ground. In most meteorite falls, the first meteorites show up on radar 90 seconds to 2 minutes after the fireball terminus, and the last (and smallest) meteorites disappear from radar about 10 minutes after the event.There are several types of radar data products, but the two most useful for finding meteorites are "Reflectivity" and "Velocity". ย
HOW TO HANDLE METEORITES
First and foremost, meteorites are not harmful to humans or to any terrestrial life. Meteorite handling procedures are designed to protect the meteorite from terrestrial contamination and alteration, not to protect people from meteorites. The goal of proper meteorite handling is to minimize harm to the meteorites to preserve their scientific and aesthetic qualities.
ย WHAT TO DO
Collect and handle meteorites using clean gloves, tongs, or new aluminum foil. Common, household aluminum foil is a reasonable and inexpensive means to handle meteorites. Simply tear a fresh piece of foil off of the roll and pick up the meteorite with it. You can keep the foil wrapped around the meteorite indefinitely.
Keep the meteorite clean and dry. You can place it in a zip-lock bag to offer it a measure of protection against atmospheric humidity. Moisture absorption packages are beneficial as well. If you use one of these, place it in the bag but keep it out of direct contact with the meteorite. Keep the meteorite wrapped in aluminum foil, place a dessicant package in the bag with it, and keep it sealed.
ย WHAT NOT TO DO
Try not to handle any freshly fallen meteorites with your bare hands! Oils and microbes from your skin will slowly degrade the surface of a meteorite, dulling the fusion crust, contaminating the meteorite, and promoting rust. The contamination aspect is especially important for carbonaceous meteorites and other uncommon types.ย
Near Earth Objects (NEO)
The following table lists all the known upcoming approaches with Near Earth Objects (NEO's) that will be closer than 20 turns around the Earth and will happen in the next 10 years. Distances are provided in km and Astronomical Units (AU):ย
Interesting Facts:
Age: The oldest particles found in meteorites, called calcium-aluminum-rich inclusions, are estimated to be 4.56 billion years old, nearly as old as our solar system!
Origin: Most meteorites come from shattered asteroids, but some originate from the Moon or Mars. There's even a possibility of material from Mercury or Venus reaching Earth, although none have been definitively identified yet.
Composition: Meteorites come in three main types:
Stony meteorites (most common): Composed mainly of silicate minerals like rock.
Iron meteorites: Largely made of iron and nickel.
Stony-iron meteorites: A blend of rock and metal.
Scientific Importance: Meteorites offer valuable clues about the formation of our solar system and the early conditions that existed. They can also contain organic compounds, raising questions about the origins of life on Earth.
Most Valuable Meteorites Ever Sold
ย The Fukang Meteorite
ย Price:ย โฌ 1 654 00
ย Landed: Fukang, China
ย Material: Iron pallasite, olivine
ย Found: 2000
ย Willamette Meteorite
ย Price: โฌ 1 300 000
ย Landed: Clackamas County, Oregon
ย Material: Iron, medium octahedrite
ย Found: Unknown
Brenham Meteorite
ย Price: โฌ 871 000
ย Landed: Kiowa County, Kansas
ย Material: Iron anomalous pallasite
ย Found: 1882
The Conception Junction Meteorite
ย Price: โฌ 703 000
ย Landed: Conception Junction, Missouri
ย Material: Iron pallasite
ย Found: 2006
Bur-Abor, an Incomparable Meteorite Specimen
ย Price: โฌ 600 000 - โฌ 800 000
ย Landed: Kenya
ย Material: Iron
ย Found: 1997
Tisserlittine Lunar Meteorite
ย Price: โฌ 480 500
ย Landed: Sahara Dessert, Kidal, Mali
ย Material: Anorthite, Olivine, pigeonite, augite, spinel troilite
ย Found: 2019
Superb Main Mass โ Individual
ย Price: โฌ 349 000
ย Landed: Sahara desert
ย Material: Martian shergottite, chondrite
ย Found: 2018
Gibeon Meteorite
ย Price: โฌ 280 000ย
ย Landed: Great Nama Land, Namibia
ย Material: Iva iron, fine octahedrite gibeon
ย Found: 1838
Springwater Meteorite
ย Price: โฌ 80 000 - โฌ 120 000ย
ย Landed: Saskatchewan, Canada
ย Material: Stony iron pallasite, kamacite, taenite, olivine
ย Found: 1931
Asteroid 16 Psyche - โฌ 10 quadrillion (that's a 10 with 15 zeros after it!).ย
enough to give everyone on Earth โฌ 1,25 billion.
The value based on current market of the materials prices (2024) and the high potential scientific value due to its likely composition. This is an hypothetical scenario even cos observations only mention the dominance of iron and nickel, the exact composition and the presence of other elements remain uncertain.
The upcoming Psyche mission aims to gather more detailed data and improve our understanding of this unique asteroid.ย
it's important to remember the practical and economic limitations of asteroid mining.
Conspiracy theorie :ย The multibillionaires, through extravagance even in the form of thoughts or the simple fact of the singularity not only of the asteroid, and also of the event itself, are already becoming even richer with the minerals contained in it and no one knows.
16 Psyche orbits the sun every 1,830 days (5.01 years), coming as close as 2.53 AU and reaching as far as 3.32 AU from the sun. Psyche is about 226.0 kilometers in diameter, making it slightly less than half the width of mainland Portugal at its widest point. The rotation of Psyche has been observed.ย
Size Estimation (Very Approximate):
Average Density: Assuming an average density of 8,350 kg/mยณ (average of iron and nickel densities):
This is a simplification; the actual density might vary depending on the composition.
Volume Calculation (for two scenarios):
Scenario 1 (30% Iron & Nickel): Volume = Mass / Density Volume = (2.1 x 10^19 kg) / (8,350 kg/mยณ) โ 2.52 x 10^16 mยณ
Scenario 2 (60% Iron & Nickel): Assuming a higher concentration of iron and nickel increases the density: * We can estimate a higher average density (e.g., 8,700 kg/mยณ). * New Volume = (2.1 x 10^19 kg) / (8,700 kg/mยณ) โ 2.41 x 10^16 mยณ
Diameter Estimation (Even More Approximate):
Assuming a spherical shape (might not be the case).
Using the formula for the volume of a sphere: Volume = (4/3)ฯrยณ
Solving for radius (r) and multiplying by 2 to get diameter.
Who discovered Psyche 16 and when?ย
Psyche 16 was discovered by Annibale de Gasparis, an Italian astronomer, on March 17, 1852. He was a prominent astronomer known for his contributions to theoretical astronomy and his discoveries of multiple asteroids. Interestingly, Psyche 16 was the 16th asteroid discovered, which is why it has the number "16" in its name.ย
Why was there a delay in scientists studying Psyche 16 in detail?ย
Although Psyche 16 was discovered in 1852, technological limitations at the time prevented detailed studies. In-depth scans and dedicated scientific interest likely came much later, around the late 20th or early 21st century. This delay can be attributed to several factors:
Limited Astronomical Technology: Early telescopes in the 19th century couldn't provide the resolution and data needed for comprehensive studies of distant objects like asteroids.
Shifting Priorities: Initially, astronomers focused their observations on celestial bodies closer to Earth, such as planets and more easily observable asteroids.
Later Technological Advancements: The development of more powerful telescopes, radar technology, and space exploration capabilities in the late 20th and early 21st centuries enabled scientists to gather more detailed information about Psyche 16, sparking a surge in scientific interest.
Key Space Law Principles:
The Outer Space Treaty (OST) is the foundation for international space law. It establishes several key principles that apply to Psyche 16:
Freedom of Exploration and Use: Outer space, including celestial bodies like asteroids, is free for exploration and use by all nations.
Non-Appropriation: No country can claim ownership of Psyche 16 or any other celestial body.
Peaceful Purposes: Space exploration and use must be for peaceful purposes.
Specific Regulations for Asteroids:
Currently, there are no specific international regulations regarding asteroid mining. However, the following are relevant:
The Moon Agreement: This agreement, not widely ratified, extends some principles of the OST to the Moon and other celestial bodies.
Developing Regulations: Discussions are ongoing about creating a legal framework for asteroid mining that considers resource utilization and environmental protection.
So, can anyone get the gold from Psyche 16?
Current Scenario: Based on existing laws, technically, any nation or private entity could attempt to explore and extract resources from Psyche 16, as long as they comply with the OST principles. This includes peaceful purposes and avoiding harmful interference with other space activities.
Here are some interesting aspects of Psyche 16 that you might find worth exploring:
Formation and Composition:
Unique Composition: Psyche 16, unlike most asteroids composed primarily of rock and ice, is believed to be a metallic asteroid, potentially composed of iron and nickel. This raises questions about its formation process and how it ended up in the asteroid belt.
Clues to Early Solar System: Understanding Psyche 16's composition could provide insights into the formation of planets and the early solar system. It might represent the core of a planet that never fully formed.
Scientific Mission:
NASA's Psyche Mission: This upcoming mission aims to launch in 2023 and reach Psyche 16 in 2029. The spacecraft will study the asteroid's composition, magnetic field, and surface features, providing valuable data to unlock its secrets.
Future Exploration and Potential Value:
Technological Hurdles: Currently, extracting resources from distant asteroids is not economically feasible due to technological limitations. However, advancements in space travel and resource processing could change this scenario in the distant future.
Scientific Value vs. Economic Potential: While the economic value of Psyche 16's resources is uncertain in the near future, its scientific value is undeniable. Understanding its composition can revolutionize our knowledge of planetary formation and the history of our solar system.
Here are some resources you might find helpful to learn more:
NASA's Psyche Mission website: https://www.jpl.nasa.gov/missions/psyche
Scientific articles and news about Psyche 16: You can find these by searching online using keywords like "Psyche 16 composition," "Psyche 16 formation," or "Psyche 16 NASA mission."
Additionally, here are some specific questions you might consider exploring further:
What are the different theories about how Psyche 16 formed?
What are the challenges of the Psyche mission, and how will scientists overcome them?
How could advancements in space technology change the economic viability of asteroid mining in the future?
A collision between Psyche 16 and Earth would be a cataclysmic event with devastating consequences. Here's a breakdown of the potential impacts:
Immediate Impact:
Global devastation: The impact would release an unimaginable amount of energy, likely exceeding the combined force of all nuclear weapons ever detonated. This could trigger:
Massive earthquakes and tsunamis: The impact would cause widespread seismic activity, potentially triggering megathrust earthquakes and devastating tsunamis that could inundate coastal regions.
Extreme heat: The impact would generate immense heat, potentially igniting widespread wildfires and causing significant atmospheric heating.
Loss of life: The immediate effects would likely cause widespread death and destruction on a global scale. Dust and debris would choke the atmosphere, blocking sunlight and causing a prolonged "impact winter."
Ecological disruption: The impact and its aftermath would severely disrupt ecosystems:
Plant life: Reduced sunlight could lead to widespread plant die-off, disrupting food chains.
Animal life: The disruption of ecosystems and food chains would have a cascading effect on animal populations.
Long-Term Effects:
Atmospheric changes: The impact could trigger changes in the composition and temperature of the atmosphere, potentially making it difficult for some life forms to survive.
Long-term climate effects: Dust and debris ejected into the atmosphere could block sunlight for extended periods, causing a global cooling effect.
Probability of such an Impact based on current information and what we know about the asteroid belt:
Low Probability: The vast majority of asteroids in the asteroid belt, including Psyche 16, are in stable orbits that pose no immediate threat to Earth.
Millions of Years: The probability of an asteroid the size of Psyche 16 impacting Earth is considered to be extremely low, occurring on timescales of millions of years.
While we can't provide a specific percentage chance, the scientific consensus is that Psyche 16 poses no imminent threat to Earth. Space agencies like NASA are continuously monitoring NEOs to ensure early detection and potential deflection strategies if a future threat is ever identified.ย
Planetary Defense Efforts:
Monitoring and Tracking: Space agencies like NASA track near-Earth objects (NEOs) to assess potential impact threats.
Deflection Techniques: Scientists are exploring various deflection techniques that could potentially nudge an asteroid off a collision course with Earth, if such a threat were ever identified.
While the likelihood of a Psyche 16 impact is very low, it highlights the importance of planetary defense efforts to monitor and potentially deflect future threats from asteroids and comets.
A few of the more notable meteorites recovered include Tissint and Northwest Africa 7034. Tissint was the first witnessed Martian meteorite fall in more than fifty years; NWA 7034 is the oldest meteorite known to come from Mars, and is a unique water-bearing regolith breccia.ย