Comets are icy counterparts to asteroids that formed beyond the frost line in the early solar system. They have a frozen nucleus and can grow comas and tails as they enter the inner solar system and warm. Comet showers occur when Earth crosses a comet's orbit and encounters dust ejected along its path. The Kuiper belt contains orderly comet orbits beyond Neptune, while the distant Oort cloud has randomly distributed comet orbits initially placed there by interactions with giant planets. Spacecraft images have revealed diverse geology on comet nuclei including cliffs, mesas, and circular depressions.
A comet is an icy small Solar System body (SSSB) that, when close enough to the Sun, displays a visible coma (a thin, fuzzy, temporary atmosphere) and sometimes also a tail. These phenomena are both due to the effects of solar radiation and the solar wind upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust and small rocky particles. Comets have been observed since ancient times.
Comets have a wide range of orbital periods, ranging from a few years to hundreds of thousands of years. Short-period comets originate in the Kuiper belt, or its associated scattered disc,[1] which lie beyond the orbit of Neptune. Longer-period comets are thought to originate in the Oort cloud, a hypothesized spherical cloud of icy bodies in the outer Solar System. Long-period comets plunge towards the Sun from the Oort cloud because of gravitational perturbations caused by either the massive outer planets of the Solar System (Jupiter, Saturn, Uranus, and Neptune), or passing stars. Rare hyperbolic comets pass once through the inner Solar System before being thrown out into interstellar space along hyperbolic trajectories. Exocomets, comets beyond our solar system, have also been detected and may be common in the Milky Way Galaxy.[2]
Comets are distinguished from asteroids by the presence of a coma or a tail. However, extinct comets that have passed close to the Sun many times have lost nearly all of their volatile ices and dust and may come to resemble small asteroids.[3] Asteroids are thought to have a different origin from comets, having formed inside the orbit of Jupiter rather than in the outer Solar System.[4][5] The discovery of main-belt comets and active centaurs has blurred the distinction between asteroids and comets (see asteroid terminology).
As of January 2011 there are a reported 4,185 known comets[6] of which about 1,500 are Kreutz Sungrazers and about 484 are short-period.[7] This number is steadily increasing. However, this represents only a tiny fraction of the total potential comet population: the reservoir of comet-like bodies in the outer Solar System may number one trillion.[8] The number visible to the naked eye averages roughly one per year, though many of these are faint and unspectacular.[9] Particularly bright or notable examples are called "Great Comets".
This is all about comets. Their parts, their origin, and this also have The Top 10 Famous Comets. This also have the definition of the Kuiper Belt and the Oort Cloud. Have a Blast!!!
A comet is an icy small Solar System body (SSSB) that, when close enough to the Sun, displays a visible coma (a thin, fuzzy, temporary atmosphere) and sometimes also a tail. These phenomena are both due to the effects of solar radiation and the solar wind upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust and small rocky particles. Comets have been observed since ancient times.
Comets have a wide range of orbital periods, ranging from a few years to hundreds of thousands of years. Short-period comets originate in the Kuiper belt, or its associated scattered disc,[1] which lie beyond the orbit of Neptune. Longer-period comets are thought to originate in the Oort cloud, a hypothesized spherical cloud of icy bodies in the outer Solar System. Long-period comets plunge towards the Sun from the Oort cloud because of gravitational perturbations caused by either the massive outer planets of the Solar System (Jupiter, Saturn, Uranus, and Neptune), or passing stars. Rare hyperbolic comets pass once through the inner Solar System before being thrown out into interstellar space along hyperbolic trajectories. Exocomets, comets beyond our solar system, have also been detected and may be common in the Milky Way Galaxy.[2]
Comets are distinguished from asteroids by the presence of a coma or a tail. However, extinct comets that have passed close to the Sun many times have lost nearly all of their volatile ices and dust and may come to resemble small asteroids.[3] Asteroids are thought to have a different origin from comets, having formed inside the orbit of Jupiter rather than in the outer Solar System.[4][5] The discovery of main-belt comets and active centaurs has blurred the distinction between asteroids and comets (see asteroid terminology).
As of January 2011 there are a reported 4,185 known comets[6] of which about 1,500 are Kreutz Sungrazers and about 484 are short-period.[7] This number is steadily increasing. However, this represents only a tiny fraction of the total potential comet population: the reservoir of comet-like bodies in the outer Solar System may number one trillion.[8] The number visible to the naked eye averages roughly one per year, though many of these are faint and unspectacular.[9] Particularly bright or notable examples are called "Great Comets".
This is all about comets. Their parts, their origin, and this also have The Top 10 Famous Comets. This also have the definition of the Kuiper Belt and the Oort Cloud. Have a Blast!!!
Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, cosmological, calendrical, and astrological beliefs and practices of pre-history: vestiges of these are still found in astrology, a discipline long interwoven with public and governmental astronomy, and not completely disentangled from it until a few centuries ago in the Western World (see astrology and astronomy). In some cultures, astronomical data was used for astrological prognostication.
Ancient astronomers were able to differentiate between stars and planets, as stars remain relatively fixed over the centuries while planets will move an appreciable amount during a comparatively short time.
A "lunar eclipse" and a "solar eclipse" refer to events involving three celestial bodies: the Sun ("solar"), the moon ("lunar"), and the Earth. A lunar eclipse occurs when the Earth passes between the Moon and the Sun, and the Earth's shadow obscures the moon or a portion of it. A solar eclipse occurs when the Moon passes between the Earth and the Sun, blocking all or a portion of the Sun.
Learn about comets, what they’re made of, and how they move from the university that has discovered 52% of all known near-Earth objects, including comets.
Astronomy is the oldest of the natural sciences, dating back to antiquity, with its origins in the religious, mythological, cosmological, calendrical, and astrological beliefs and practices of pre-history: vestiges of these are still found in astrology, a discipline long interwoven with public and governmental astronomy, and not completely disentangled from it until a few centuries ago in the Western World (see astrology and astronomy). In some cultures, astronomical data was used for astrological prognostication.
Ancient astronomers were able to differentiate between stars and planets, as stars remain relatively fixed over the centuries while planets will move an appreciable amount during a comparatively short time.
A "lunar eclipse" and a "solar eclipse" refer to events involving three celestial bodies: the Sun ("solar"), the moon ("lunar"), and the Earth. A lunar eclipse occurs when the Earth passes between the Moon and the Sun, and the Earth's shadow obscures the moon or a portion of it. A solar eclipse occurs when the Moon passes between the Earth and the Sun, blocking all or a portion of the Sun.
Learn about comets, what they’re made of, and how they move from the university that has discovered 52% of all known near-Earth objects, including comets.
A powerpoint presentation on comets. A comet is an icy, small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process that is called outgassing. This produces a visible atmosphere or coma, and sometimes also a tail.
What is Earth and space science about?
Earth and space science (ESS) connects systems
Earth and space science explores the interconnections between the land, ocean, atmosphere, and life of our planet. These include the cycles of water, carbon, rock, and other materials that continuously shape, influence, and sustain Earth and its inhabitants.
ESS also explores the cyclical interactions between the Earth system and the Sun and Moon.
ESS explores how New Zealand has been shaped by its location
New Zealand straddles the boundary between two major tectonic plates. ESS scientists – and students who study ESS – investigate how this precarious location has impacted (and continues to impact) on New Zealand’s geology and landforms, sometimes in dramatic ways.
ESS investigates the major ocean currents that flow past New Zealand and the impact these and other factors have on our weather and climate.
ESS explores the solar system and beyond
Planet Earth is dynamically linked with the solar system and the wider universe. ESS investigates the structure and composition of these systems and develops understanding of the vast distances and times involved.
What is the Nature of Science strand about?
Why study Earth and space science?
Key concepts: Earth and space science
What is biology | physics | chemistry about?
Interpreting the Nature of Science in an ESS context
Understanding about science
Students learn how understanding of the Earth system, the solar system, the universe, and the interactions between them has developed over time. For example, how:
Wegener and other scientists came to understand that the surface of the earth is broken into tectonic plates that move and interact at their boundaries
Pluto was discovered in 1930 because of disturbances in the orbits of Uranus and Neptune and became the ninth planet, only to be declared a dwarf planet in 2006 after the discovery of Kuiper Belt objects of similar sizes
technologies such as space telescopes and probes have facilitated a build-up of knowledge and understanding about planets, moons, and the rest of the universe
attempts by humans to travel in space have been influenced by the politics of the day
satellites that can measure such factors as the temperature of the surface of the ocean make it possible to build computer models that can be used to accurately monitor changes in the Earth system
the cumulative work of many scientific teams has led to such breakthroughs as understanding the mechanisms of climate change and ocean acidification.
Investigating in science
Students investigate aspects of the Earth system, the solar system and the universe. For example:
Investigating the exchange of carbon dioxide between the ocean and atmosphere by undertaking practical investigations and processing and interpreting secondary data.
Investigating the Sun, Moon and Earth cycles by exploring and developing different models.
useful student materials reference for basic education. Asteroids, comets, and meteors are chunks of rock, ice, and metal left over from the formation of our solar system 4.6 billion years ago. They are a lot like a fossil record of our early solar system. There are about 1.3 million known asteroids, and more than 3,800 known comets. If we take a complete inventory of the entire contents of the Solar System, we find that there are many small, rocky bodies ranging in size from similar to grains of sand up to the size of small moons or comets. The smallest rocky objects that are found in space are referred to as meteoroids. There are three different classifications of meteoroids, depending on how they are observed:
Meteoroid: A chunk of rock orbiting the Sun inside the Solar System.
Meteor: When a meteoroid encounters the Earth's atmosphere, it interacts with the gases in the atmosphere and all or most of it gets vaporized. The streak of light that we see as the rock penetrates the atmosphere is called a meteor, which many people refer to as "a shooting star."
Meteorite: If some of the material that makes up a meteoroid survives the trip through the atmosphere and is found on Earth, we refer to the remnant as a meteorite. If you want help identifying candidate meteorites you can see the following page:
University of New Mexico: How to Identify a Meteorite(link is external)
There are many meteorites that have been recovered on Earth. We find that there are several types of meteorites that can be separated based on their composition. Some meteorites are almost entirely made up of iron and nickel. These chunks of metal are very easy to find when they land on the Earth because they are so dense and are essentially chunks of metal. There are also stone and stony-iron mix meteorites that land on the Earth (these are more common), but since they appear to the untrained eye more like the naturally occurring rocks on the Earth, without extensive testing they are more difficult to identify as meteorites. During its mission, the Mars Rover Opportunity discovered an iron meteorite on Mars. It just happened to be lying on the planet's surface right near where the Rover's heat shield landed after the spacecraft jettisoned it. This is an iron meteorite, making it stand out among the other rocks the Rover has studied intensively during its trip around the surface of Mars.
Astronomy - State of the Art - ExoplanetsChris Impey
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the dramatic discoveries of exoplanets or extra-solar planets are discussed.
Instructions for Submissions thorugh G- Classroom.pptxJheel Barad
This presentation provides a briefing on how to upload submissions and documents in Google Classroom. It was prepared as part of an orientation for new Sainik School in-service teacher trainees. As a training officer, my goal is to ensure that you are comfortable and proficient with this essential tool for managing assignments and fostering student engagement.
Synthetic Fiber Construction in lab .pptxPavel ( NSTU)
Synthetic fiber production is a fascinating and complex field that blends chemistry, engineering, and environmental science. By understanding these aspects, students can gain a comprehensive view of synthetic fiber production, its impact on society and the environment, and the potential for future innovations. Synthetic fibers play a crucial role in modern society, impacting various aspects of daily life, industry, and the environment. ynthetic fibers are integral to modern life, offering a range of benefits from cost-effectiveness and versatility to innovative applications and performance characteristics. While they pose environmental challenges, ongoing research and development aim to create more sustainable and eco-friendly alternatives. Understanding the importance of synthetic fibers helps in appreciating their role in the economy, industry, and daily life, while also emphasizing the need for sustainable practices and innovation.
We all have good and bad thoughts from time to time and situation to situation. We are bombarded daily with spiraling thoughts(both negative and positive) creating all-consuming feel , making us difficult to manage with associated suffering. Good thoughts are like our Mob Signal (Positive thought) amidst noise(negative thought) in the atmosphere. Negative thoughts like noise outweigh positive thoughts. These thoughts often create unwanted confusion, trouble, stress and frustration in our mind as well as chaos in our physical world. Negative thoughts are also known as “distorted thinking”.
Read| The latest issue of The Challenger is here! We are thrilled to announce that our school paper has qualified for the NATIONAL SCHOOLS PRESS CONFERENCE (NSPC) 2024. Thank you for your unwavering support and trust. Dive into the stories that made us stand out!
Students, digital devices and success - Andreas Schleicher - 27 May 2024..pptxEduSkills OECD
Andreas Schleicher presents at the OECD webinar ‘Digital devices in schools: detrimental distraction or secret to success?’ on 27 May 2024. The presentation was based on findings from PISA 2022 results and the webinar helped launch the PISA in Focus ‘Managing screen time: How to protect and equip students against distraction’ https://www.oecd-ilibrary.org/education/managing-screen-time_7c225af4-en and the OECD Education Policy Perspective ‘Students, digital devices and success’ can be found here - https://oe.cd/il/5yV
How to Make a Field invisible in Odoo 17Celine George
It is possible to hide or invisible some fields in odoo. Commonly using “invisible” attribute in the field definition to invisible the fields. This slide will show how to make a field invisible in odoo 17.
Unit 8 - Information and Communication Technology (Paper I).pdfThiyagu K
This slides describes the basic concepts of ICT, basics of Email, Emerging Technology and Digital Initiatives in Education. This presentations aligns with the UGC Paper I syllabus.
The Art Pastor's Guide to Sabbath | Steve ThomasonSteve Thomason
What is the purpose of the Sabbath Law in the Torah. It is interesting to compare how the context of the law shifts from Exodus to Deuteronomy. Who gets to rest, and why?
Model Attribute Check Company Auto PropertyCeline George
In Odoo, the multi-company feature allows you to manage multiple companies within a single Odoo database instance. Each company can have its own configurations while still sharing common resources such as products, customers, and suppliers.
2. 1515
GoalsGoals
• What are comets?
• How are they different from asteroids?
• What are meteor showers?
• How are they different from typical meteors?
3. 1515
Comets – Hale Bopp
Copyright – Tyler Nordgren
Copyright – Tyler Nordgren
Copyright – John Glerason
5. 1515
Comet Facts
• Formed beyond the frostline, comets are icy
counterparts to asteroids.
• “Dirty snowballs” = the nucleus
• Most comets do not have tails.
• Most comets remain perpetually frozen in the
outer solar system. Only a few enter the inner
solar system, where they can grow tails.
7. 1515
Concept Test
• Suppose we discover a new comet on an
orbit that brings it closer to the Sun than
Mercury every 125 years. What can we
conclude?
a. It has been on its current orbit for only a very
short time compared to the age of our solar
system.
b. It has a coma and tail during most of each orbit.
c. It came from the Oort cloud.
d. It came from the Kuiper belt.
e. None of the above.
9. 1515
Concept Test
• Why are comets icier than asteroids?
a. Asteroids were once as icy but the solar wind
blasted it away
b. Planetesimals that formed closer to the Sun
contained fewer ices
c. The sun’s gravity attracts dense objects more
d. Comets and asteroids formed in the same region
but asteroids were flung outward
e. Comets are not icier: comets are actually less icy
on average
11. 1515
Concept Test
• Suppose there were no solar wind. How
would the appearance of a comet in our
inner solar system be different?
a. It would not have an ion tail.
b. It would not have a nucleus.
c. It would not have a coma.
d. It would be much brighter in appearance.
e. It would not have a dust tail.
16. 1515
Kuiper belt:
On orderly orbits
from 30-100 AU in
disk of solar
system
Oort cloud:
On random orbits
extending to about
50,000 AU
Only a tiny number
of comets enter the
inner solar system -
most stay far from
the Sun
18. 1515
How did they get there?
• Kuiper belt comets formed in the Kuiper belt: flat
plane, aligned with the plane of planetary orbits,
orbiting in the same direction as the planets.
• Oort cloud comets were once closer to the Sun, but
they were kicked out there by gravitational
interactions with jovian planets: spherical
distribution, orbits in any direction.
19. 1515
Concept Test
• Oort cloud comet orbits are ‘random’ compared to
Kuiper Belt comets because…
a. The comets have collided so frequently their orbits became
randomized
b. They formed from the collapsing cloud before it formed an
organized disk
c. They were ejected by the jovian planets onto random orbits
d. Orbital resonances with nearby stars randomized the
orbits
e. None of the above: Kuiper Belt comets have more random
orbits
20. 1515
Halley Borrelly Wild 2
• Mesas
• “Craters” (circular depressions)
• “Smooth” terrain as sources of jets
• Pinnacles
• Dark Spots; Bright Spots (small albedo features)
• Sharp Edges
Each nucleus had some (but not all!) of these:
21. 1515
Deep Impact
• NASA mission to impact comet nucleus.
• Use spectroscopy to determine composition
of nucleus.
Deep Impact movies
23. 1515A’Hearn et al 2005
Geology of theGeology of the
surfacesurface
• Circular “craters”: due
to impacts? Like Wild 2?
Unlike Borrelly.
• Cliffs, mesas: like
Borrelly, maybe like Wild
2.
• Smooth and rough
terrains, like Borrelly.
• Fairly uniform
reflectivity, like Wild 2,
unlike Borrelly.