• The term LD stands for Lunar Distance, which is a unit of measurement used in astronomy to express the distance between the Earth and the Moon. One LD is approximately 384,400 kilometers (or about 238,855 miles), the average distance from the Earth to the Moon.

    When discussing asteroid distances in terms of LD, it indicates how far the asteroid is from Earth relative to the Moon's distance. For example:

    0.5 LD means the asteroid is half the distance from the Earth to the Moon (about 192,200 kilometers).
    1 LD means the asteroid is at the same average distance as the Moon.
    10 LD means the asteroid is ten times farther away than the Moon's average distance.
    Why is LD used for asteroids?
    Using LD is a convenient way to quickly understand the proximity of asteroids to Earth, especially for Near-Earth Objects (NEOs). It provides a clear, relatable frame of reference since the Moon is a familiar benchmark.

    For instance:

    An asteroid passing at 0.1 LD (about 38,440 kilometers) is considered a very close approach.
    An asteroid at 5 LD (1,922,000 kilometers) is farther but still monitored, depending on its size and trajectory.
    The term LD stands for Lunar Distance, which is a unit of measurement used in astronomy to express the distance between the Earth and the Moon. One LD is approximately 384,400 kilometers (or about 238,855 miles), the average distance from the Earth to the Moon. When discussing asteroid distances in terms of LD, it indicates how far the asteroid is from Earth relative to the Moon's distance. For example: 0.5 LD means the asteroid is half the distance from the Earth to the Moon (about 192,200 kilometers). 1 LD means the asteroid is at the same average distance as the Moon. 10 LD means the asteroid is ten times farther away than the Moon's average distance. Why is LD used for asteroids? Using LD is a convenient way to quickly understand the proximity of asteroids to Earth, especially for Near-Earth Objects (NEOs). It provides a clear, relatable frame of reference since the Moon is a familiar benchmark. For instance: An asteroid passing at 0.1 LD (about 38,440 kilometers) is considered a very close approach. An asteroid at 5 LD (1,922,000 kilometers) is farther but still monitored, depending on its size and trajectory.
    0 Комментарии 0 Поделились 379 Просмотры
  • The Vega star system is one of the most studied in astronomy due to its proximity, brightness, and unique characteristics that challenge our understanding of planet formation and stellar evolution. Located just 25 light-years away from Earth in the constellation Lyra, Vega is a blue-white star and the fifth-brightest star visible in our night sky. Here's a breakdown of the most intriguing features of the Vega system:

    1. Dust Disk Discovery
    Infrared Excess: In the 1980s, the Infrared Astronomical Satellite (IRAS) discovered an excess of infrared radiation from Vega, indicating a dust disk around the star. This disk emits infrared radiation as dust particles are heated by Vega's light, suggesting an early model of a protoplanetary or debris disk.
    Smooth Disk: Unlike other systems like Fomalhaut, Vega’s disk is remarkably smooth, lacking the gaps and rings typically associated with planets disturbing the dust. This smoothness implies that Vega may lack substantial planetary influences or that planets there may be few and more challenging to detect.
    2. Potential "Hot Neptune"
    Astronomers have hypothesized that Vega might host a hot Neptune—a large planet orbiting close to the star, with a mass similar to that of Uranus or Neptune. If present, this planet could slightly perturb the disk, though not enough to create the pronounced structures seen in other systems.
    3. Asteroid Belt Analogy
    Collapse
    Observations suggest that Vega may contain a large asteroid belt similar to our Solar System's, with a spread-out disk of rocky material. This possible asteroid belt might add to the dust observed around Vega and could provide insights into the early formation phases of planetary systems.
    4. Historical and Cultural Significance
    Former Pole Star: Around 14,000 years ago, Earth's axis pointed toward Vega, making it the northern pole star until approximately 12,000 BC. The star held great significance for ancient civilizations due to its prominence.
    Name and Mythology: The name "Vega," originally spelled "Wega," comes from the Arabic "Al Nasr al Waki," meaning "Swooping Eagle." Vega is a cornerstone of the Summer Triangle, a prominent asterism for northern hemisphere skywatchers, along with Altair and Deneb.
    5. Milestones in Astronomy
    First Stellar Spectrum: Vega was the first star to have its spectrum recorded in 1850, helping astronomers study stellar composition and temperature.
    Early Photographic Milestone: It was also the second star, after the Sun, to be photographed, marking a major step in astronomical imaging.
    6. Variable Star Characteristics
    Vega is classified as a Delta Scuti variable, with slight pulsations that cause small changes in its brightness over time. Although minimal, these fluctuations provide valuable data for stellar research and challenge Vega's historic role as a "constant" in brightness.
    7. Future Research and Exploration
    With its dust disk and potential hot Neptune, Vega remains a prime target for studying alternative pathways in planetary system evolution. Optical spectroscopy allows astronomers to analyze parameters such as star formation rates and chemical composition, shedding light on the processes within Vega's disk and its potential for planet formation.
    8. Vega's characteristics—its smooth disk, possible planetary companions, and cultural prominence—continue to intrigue astronomers. Future missions and telescopes may reveal more about this iconic star system, potentially uncovering planets or additional features that reshape our understanding of how stars and planetary systems evolve.
    The Vega star system is one of the most studied in astronomy due to its proximity, brightness, and unique characteristics that challenge our understanding of planet formation and stellar evolution. Located just 25 light-years away from Earth in the constellation Lyra, Vega is a blue-white star and the fifth-brightest star visible in our night sky. Here's a breakdown of the most intriguing features of the Vega system: 1. Dust Disk Discovery Infrared Excess: In the 1980s, the Infrared Astronomical Satellite (IRAS) discovered an excess of infrared radiation from Vega, indicating a dust disk around the star. This disk emits infrared radiation as dust particles are heated by Vega's light, suggesting an early model of a protoplanetary or debris disk. Smooth Disk: Unlike other systems like Fomalhaut, Vega’s disk is remarkably smooth, lacking the gaps and rings typically associated with planets disturbing the dust. This smoothness implies that Vega may lack substantial planetary influences or that planets there may be few and more challenging to detect. 2. Potential "Hot Neptune" Astronomers have hypothesized that Vega might host a hot Neptune—a large planet orbiting close to the star, with a mass similar to that of Uranus or Neptune. If present, this planet could slightly perturb the disk, though not enough to create the pronounced structures seen in other systems. 3. Asteroid Belt Analogy Collapse Observations suggest that Vega may contain a large asteroid belt similar to our Solar System's, with a spread-out disk of rocky material. This possible asteroid belt might add to the dust observed around Vega and could provide insights into the early formation phases of planetary systems. 4. Historical and Cultural Significance Former Pole Star: Around 14,000 years ago, Earth's axis pointed toward Vega, making it the northern pole star until approximately 12,000 BC. The star held great significance for ancient civilizations due to its prominence. Name and Mythology: The name "Vega," originally spelled "Wega," comes from the Arabic "Al Nasr al Waki," meaning "Swooping Eagle." Vega is a cornerstone of the Summer Triangle, a prominent asterism for northern hemisphere skywatchers, along with Altair and Deneb. 5. Milestones in Astronomy First Stellar Spectrum: Vega was the first star to have its spectrum recorded in 1850, helping astronomers study stellar composition and temperature. Early Photographic Milestone: It was also the second star, after the Sun, to be photographed, marking a major step in astronomical imaging. 6. Variable Star Characteristics Vega is classified as a Delta Scuti variable, with slight pulsations that cause small changes in its brightness over time. Although minimal, these fluctuations provide valuable data for stellar research and challenge Vega's historic role as a "constant" in brightness. 7. Future Research and Exploration With its dust disk and potential hot Neptune, Vega remains a prime target for studying alternative pathways in planetary system evolution. Optical spectroscopy allows astronomers to analyze parameters such as star formation rates and chemical composition, shedding light on the processes within Vega's disk and its potential for planet formation. 8. Vega's characteristics—its smooth disk, possible planetary companions, and cultural prominence—continue to intrigue astronomers. Future missions and telescopes may reveal more about this iconic star system, potentially uncovering planets or additional features that reshape our understanding of how stars and planetary systems evolve.
    0 Комментарии 0 Поделились 2Кб Просмотры
  • Mercury, the closest planet to the Sun, has been heavily bombarded by meteorites throughout its history, similar to other rocky planets in our solar system. Its surface is covered with impact craters, some of which are quite large and ancient. Due to Mercury’s lack of a significant atmosphere, incoming meteorites do not burn up, resulting in frequent and intense impacts. Notable examples include:

    Caloris Basin: One of the largest known impact craters in the solar system, the Caloris Basin spans about 1,550 kilometers (960 miles). It was likely formed by an asteroid impact during Mercury's early history.

    Kuiper Crater: A relatively small but well-preserved crater, named after the astronomer Gerard Kuiper, is about 60 kilometers (37 miles) in diameter.

    Hokusai Crater: Another large crater on Mercury, measuring 114 kilometers (71 miles) in diameter, with bright rays of ejected material extending over much of the planet.

    Mercury's surface is thought to have experienced more impacts than Earth's, Mars', or Venus' due to its proximity to the Sun, which pulls in more meteoroids and comets. These impacts have significantly shaped the planet's geological history and surface evolution.

    Tonynetone
    Mercury, the closest planet to the Sun, has been heavily bombarded by meteorites throughout its history, similar to other rocky planets in our solar system. Its surface is covered with impact craters, some of which are quite large and ancient. Due to Mercury’s lack of a significant atmosphere, incoming meteorites do not burn up, resulting in frequent and intense impacts. Notable examples include: Caloris Basin: One of the largest known impact craters in the solar system, the Caloris Basin spans about 1,550 kilometers (960 miles). It was likely formed by an asteroid impact during Mercury's early history. Kuiper Crater: A relatively small but well-preserved crater, named after the astronomer Gerard Kuiper, is about 60 kilometers (37 miles) in diameter. Hokusai Crater: Another large crater on Mercury, measuring 114 kilometers (71 miles) in diameter, with bright rays of ejected material extending over much of the planet. Mercury's surface is thought to have experienced more impacts than Earth's, Mars', or Venus' due to its proximity to the Sun, which pulls in more meteoroids and comets. These impacts have significantly shaped the planet's geological history and surface evolution. Tonynetone
    0 Комментарии 0 Поделились 1Кб Просмотры
  • Uranus, the most distant naked-eye object in the Solar System, that has seen by visible to the naked to human eye anyway visible to the naked eye, but it was not discovered in ancient times. So what's going on with this solar system planet?.

    Discovery by Telescope: Uranus was not officially recognized as a planet until 1781 when astronomer William Herschel observed it through a telescope. Herschel initially thought it was a comet, but after further observation, it became clear that it was a new planet. This was the first planet discovered with a telescope, marking the shift in how we observe the cosmos.

    Uranus is an example of how astronomical discoveries can be overlooked despite being theoretically visible for centuries, largely due to human perception, observational limitations, and the planet's peculiar characteristics. In astronomy, the naked eye may be used to observe celestial events and objects visible without equipment, such as conjunctions, passing comets, meteor showers, and the brightest asteroids., Sky lore and various tests demonstrate an impressive variety of phenomena visible to the unaided eye.
    Uranus, the most distant naked-eye object in the Solar System, that has seen by visible to the naked to human eye anyway visible to the naked eye, but it was not discovered in ancient times. So what's going on with this solar system planet?. Discovery by Telescope: Uranus was not officially recognized as a planet until 1781 when astronomer William Herschel observed it through a telescope. Herschel initially thought it was a comet, but after further observation, it became clear that it was a new planet. This was the first planet discovered with a telescope, marking the shift in how we observe the cosmos. Uranus is an example of how astronomical discoveries can be overlooked despite being theoretically visible for centuries, largely due to human perception, observational limitations, and the planet's peculiar characteristics. In astronomy, the naked eye may be used to observe celestial events and objects visible without equipment, such as conjunctions, passing comets, meteor showers, and the brightest asteroids., Sky lore and various tests demonstrate an impressive variety of phenomena visible to the unaided eye.
    0 Комментарии 0 Поделились 1Кб Просмотры
  • 2024 PT5 is indeed an intriguing near-Earth object (NEO) that falls under the Arjuna asteroid class, which is known for Earth-like orbits and slow close encounters with our planet. These types of asteroids are of special interest to astronomers because their orbits are very similar to Earth's, leading to the potential for close approaches, though they typically do not pose an immediate impact threat. The Arjuna class itself is a subset of the Apollo group, characterized by orbits that cross Earth's orbit but have longer periods.

    The discovery of 2024 PT5 by the ATLAS program at the South African Astronomical Observatory adds to our growing catalog of NEOs. The ATLAS program is part of ongoing efforts to identify and track asteroids that could come close to Earth. Due to 2024 PT5's slow passes, it is particularly useful for studying the dynamics of asteroids in Earth's vicinity.
    2024 PT5 is indeed an intriguing near-Earth object (NEO) that falls under the Arjuna asteroid class, which is known for Earth-like orbits and slow close encounters with our planet. These types of asteroids are of special interest to astronomers because their orbits are very similar to Earth's, leading to the potential for close approaches, though they typically do not pose an immediate impact threat. The Arjuna class itself is a subset of the Apollo group, characterized by orbits that cross Earth's orbit but have longer periods. The discovery of 2024 PT5 by the ATLAS program at the South African Astronomical Observatory adds to our growing catalog of NEOs. The ATLAS program is part of ongoing efforts to identify and track asteroids that could come close to Earth. Due to 2024 PT5's slow passes, it is particularly useful for studying the dynamics of asteroids in Earth's vicinity.
    0 Комментарии 0 Поделились 857 Просмотры
  • WE ARE SCIENTISTS: Scientist Without Degree Possible?
    Based on the search results, it is possible to be a scientist without a degree. Here are some key points:

    In bioinformatics, many people working in the field did not have a degree in bioinformatics until recently, when degree programs were established. Self-study and learning by doing can be sufficient to become a bioinformaticist.
    In data science, it is possible to become a data scientist without a degree, as long as one has the necessary skills and can demonstrate their abilities through work and publications.
    In programming, one can learn by self-study and experience, as exemplified by the individual who taught themselves assembly language and went on to start a company and work at Microsoft.
    In astronomy, amateur astronomers have discovered comets and asteroids, and those with larger instruments have discovered supernovae in distant galaxies, demonstrating that non-degree holders can contribute to scientific discoveries.
    The scientific community values results and replicable experiments over formal education. As long as one’s work is well-documented and replicable, their credentials will not appear on the article, and their findings will be acknowledged.
    However, it’s important to note that:

    Without a degree, it may be more challenging to gain recognition and acceptance within the scientific community, particularly in fields with strong academic traditions.
    Self-study and learning by doing require significant dedication and effort, and may not provide the same level of formal training and mentorship as a degree program.
    In some fields, such as academia or research institutions, a degree may be a requirement for employment or funding.
    Ultimately, becoming a scientist without a degree requires a strong passion for learning, a willingness to put in the effort to develop necessary skills, and a focus on producing high-quality work that can be replicated and validated by others.
    WE ARE SCIENTISTS: Scientist Without Degree Possible? Based on the search results, it is possible to be a scientist without a degree. Here are some key points: In bioinformatics, many people working in the field did not have a degree in bioinformatics until recently, when degree programs were established. Self-study and learning by doing can be sufficient to become a bioinformaticist. In data science, it is possible to become a data scientist without a degree, as long as one has the necessary skills and can demonstrate their abilities through work and publications. In programming, one can learn by self-study and experience, as exemplified by the individual who taught themselves assembly language and went on to start a company and work at Microsoft. In astronomy, amateur astronomers have discovered comets and asteroids, and those with larger instruments have discovered supernovae in distant galaxies, demonstrating that non-degree holders can contribute to scientific discoveries. The scientific community values results and replicable experiments over formal education. As long as one’s work is well-documented and replicable, their credentials will not appear on the article, and their findings will be acknowledged. However, it’s important to note that: Without a degree, it may be more challenging to gain recognition and acceptance within the scientific community, particularly in fields with strong academic traditions. Self-study and learning by doing require significant dedication and effort, and may not provide the same level of formal training and mentorship as a degree program. In some fields, such as academia or research institutions, a degree may be a requirement for employment or funding. Ultimately, becoming a scientist without a degree requires a strong passion for learning, a willingness to put in the effort to develop necessary skills, and a focus on producing high-quality work that can be replicated and validated by others.
    Love
    1
    0 Комментарии 0 Поделились 1Кб Просмотры
  • the latest spacecraft bepi colombo under threat propulsion engineers could risk its ability to complete its upcoming gravity assist. Are designed to study Mercury’s and asteroids path long-standing questions on the formation and evolution of our Solar System.
    the latest spacecraft bepi colombo under threat propulsion engineers could risk its ability to complete its upcoming gravity assist. Are designed to study Mercury’s and asteroids path long-standing questions on the formation and evolution of our Solar System.
    0 Комментарии 0 Поделились 1Кб Просмотры
  • Surprisingly NASA errors with asteroid Dimorphos the debris could hit Mars after creating debris that could pose a threat to other celestial bodies, including Mars. This scenario underscores the complexity of space missions.
    Surprisingly NASA errors with asteroid Dimorphos the debris could hit Mars after creating debris that could pose a threat to other celestial bodies, including Mars. This scenario underscores the complexity of space missions.
    0 Комментарии 0 Поделились 549 Просмотры
  • Episode 321 - A FIST FULL OF TREMORS - Clyde Lewis Ground Zero
    https://www.spreaker.com/user/aftermathfm/633736695-groundzeromedia-a-fist-full-of?mc_cid=73e102c4c0&mc_eid=5c932d9c99
    In its 4.5 billion–year history, life on Earth has been almost erased at least half a dozen times; shattered by asteroid impacts, entombed in ice, smothered by methane, and torn apart by unfathomably powerful megavolcanoes.Every day we take most disasters in stride because they are expected on a planet that is never quiet.Scientists and journalists make the simplest of scientific concepts sound incredibly complicated. They have also set agendas that approximate the arguments for climate change and hope that you forget that it was once called global warming. The media is also banking on the ignorance of the populace when they try and blame earthquakes and volcanic activity on climate.Simple differences between climate, weather, geophysical studies, and seismology have been blurred in a way that there should be a new scientific nomenclature where we can lump it all together.

    originally Broadcast On 6/7/19
    Episode 321 - A FIST FULL OF TREMORS - Clyde Lewis Ground Zero https://www.spreaker.com/user/aftermathfm/633736695-groundzeromedia-a-fist-full-of?mc_cid=73e102c4c0&mc_eid=5c932d9c99 In its 4.5 billion–year history, life on Earth has been almost erased at least half a dozen times; shattered by asteroid impacts, entombed in ice, smothered by methane, and torn apart by unfathomably powerful megavolcanoes.Every day we take most disasters in stride because they are expected on a planet that is never quiet.Scientists and journalists make the simplest of scientific concepts sound incredibly complicated. They have also set agendas that approximate the arguments for climate change and hope that you forget that it was once called global warming. The media is also banking on the ignorance of the populace when they try and blame earthquakes and volcanic activity on climate.Simple differences between climate, weather, geophysical studies, and seismology have been blurred in a way that there should be a new scientific nomenclature where we can lump it all together. originally Broadcast On 6/7/19
    0 Комментарии 0 Поделились 8Кб Просмотры
  • Katherine Kretke - NASA’s Lucy Spacecraft Discovers 2nd Asteroid During Dinkinesh Flyby:

    https://www.nasa.gov/image-article/nasas-lucy-spacecraft-discovers-2nd-asteroid-during-dinkinesh-flyby/

    #Dinkinesh #AsteroidBelt #BinaryAsteroid #Asteroid #Lucy #LORRI #NASA #SolarSystemScience #Astronomy
    Katherine Kretke - NASA’s Lucy Spacecraft Discovers 2nd Asteroid During Dinkinesh Flyby: https://www.nasa.gov/image-article/nasas-lucy-spacecraft-discovers-2nd-asteroid-during-dinkinesh-flyby/ #Dinkinesh #AsteroidBelt #BinaryAsteroid #Asteroid #Lucy #LORRI #NASA #SolarSystemScience #Astronomy
    WWW.NASA.GOV
    NASA’s Lucy Spacecraft Discovers 2nd Asteroid During Dinkinesh Flyby
    On Nov. 1, NASA’s Lucy spacecraft flew by not just its first asteroid, but its first two. The first images returned by Lucy reveal that the small main belt asteroid Dinkinesh is actually a binary pair.
    Like
    1
    0 Комментарии 0 Поделились 4Кб Просмотры
Расширенные страницы
Спонсоры

We are 100% funded for October.

Thanks to everyone who helped out. 🥰

Xephula monthly operating expenses for 2024 - Server: $143/month - Backup Software: $6/month - Object Storage: $6/month - SMTP Service: $10/month - Stripe Processing Fees: ~$10/month - Total: $175/month

Xephula Funding Meter

Please Donate Here