The Planet 9 in the Outer Solar System
- April 22, 2024
Introduction



Evidence Of A Massive Object Beyond The Orbit Of Neptune and the solar system’s distant reaches exhibit a wealth of anomalous dynamical structure. NASA researchers have found mathematical evidence suggesting there may be a "Planet X" deep in the solar system.

The outer reaches of our solar system, beyond the orbit of Neptune, are home to a vast number of trans-Neptunian objects (TNOs). These are generally small, icy bodies that orbit the sun at distances greater than 30 astronomical units (AU), where one AU is the average distance between Earth and the sun. Over 3,000 TNOs have been identified, including dwarf planets like Pluto and Eris, as well as smaller Kuiper Belt objects. These objects are far enough from Neptune that its gravity doesn't significantly affect them; instead, they're mostly tied to the solar system by the distant pull of the sun.



Anomalies in the Outer Solar System


Interestingly, the orbits of some of these TNOs exhibit anomalous structures, hinting at the presence of a yet-undetected, massive trans-Neptunian body, often referred to as Planet 9. For instance, a group of extreme trans-Neptunian objects (ETNOs), bodies that orbit the Sun at distances averaging more than 250 times that of the Earth, show peculiar clustering of orbits. These ETNOs tend to make their closest approaches to the Sun in one sector, and their orbits are similarly tilted. These alignments suggest that an undiscovered planet may be shepherding the orbits of the most distant known Solar System objects.



The Planet 9 Hypothesis


The Planet 9 hypothesis proposes the existence of a massive planet beyond Neptune that could explain these unusual orbital alignments. This hypothetical planet, if it exists, is believed to be a super-Earth or ice giant, 2 to 15 times the mass of the Earth and beyond 200 AU, possibly with a highly inclined orbit at some 1,500 AU. However, it's important to note that this is still a hypothesis, and the existence of Planet 9 has not been confirmed.



Alternative Explanations


While the Planet 9 hypothesis is compelling, it's not the only explanation for the observed anomalies. Some researchers have proposed that the gravitational influence of a massive, extended disc beyond Neptune could account for the peculiar orbits of some TNOs. This model suggests that the combined action of the giant outer planets and this disc could explain the spatially clustered orbits of some TNOs.



Conclusion


In conclusion, the anomalous dynamical structures observed in the orbits of trans-Neptunian objects hint at the presence of a yet-undetected, massive body beyond Neptune, often referred to as Planet 9. However, this remains a hypothesis, and alternative explanations, such as the influence of a massive, extended disc beyond Neptune, have also been proposed. Further observations and studies are needed to confirm or refute these theories. The mathematical calculation of a planets could explain the unique orbits of some smaller objects in the Kuiper Belt, a distant region of icy debris that extends far beyond the orbit of Neptune.

Extraterrestrial Life and the Search for Aliens
Search for extraterrestrial life,new paper suggests Aliens Already have engeignerez others planet beyond our solar system.

The paper argues that searching for these types of techno signatures could be more promising than just looking for direct communication signals from alien civilizations. The authors note that even an advanced alien civilization may not be actively trying to contact us, but they may still inadvertently leave behind detectable evidence of their presence and technological capabilities.

Overall, the paper proposes an intriguing new approach to the search for extraterrestrial intelligence (SETI) that focuses on identifying potential signs of alien-engineered planetary systems rather than just radio signals. The authors hope this will open up new avenues for discovering advanced life elsewhere in the universe.

The search for extraterrestrial life is not limited to our own solar system. Scientists have been studying exoplanets, which are planets that orbit stars outside of our solar system. The discovery of exoplanets has expanded our understanding of the potential for life beyond Earth. However, it is important to note that our knowledge of exoplanets is still limited, and we are only beginning to explore their potential habitability.

Critically évaluation the sources and evidence to ensure their reliability. Extraordinary claims require extraordinary evidence, and the Worldwide research community carefully scrutinizes such claims to ensure the integrity of the new History and Civilization about this Planet.

W1935, a brown dwarf
known as W1935 is more massive than Jupiter, and exhibited infrared emissions from methane — a finding that has puzzled scientists due to the brown dwarf's cold nature and lack of a host star to provide energy for such atmospheric phenomena.

W1935, a brown dwarf located 47 light-years from Earth, has intrigued astronomers with its unexpected behavior. Despite being more massive than Jupiter and lacking a host star, it exhibits infrared emissions from methane in its upper atmosphere. This phenomenon is puzzling because the brown dwarf is cold and lacks an obvious energy source to fuel such atmospheric processes

On Earth, aurorae are created when energetic particles from the Sun interact with our magnetic field, producing captivating curtains of light near the poles. Similarly, Jupiter and Saturn have auroral processes, including contributions from their active moons like Io and Enceladus. However, for isolated brown dwarfs like W1935, the absence of a stellar wind complicates the explanation for the extra energy needed to produce methane glow. Scientists speculate that internal processes or interactions with interstellar plasma or nearby active moons may play a role in this intriguing phenomenon.

The discovery of methane emission on W1935 is akin to a fascinating detective story, unraveling the mysteries of celestial phenomena.

Mysterious aurora over 'failed star' 'shocking' discovery that transformed into pure fantasy the astrophysics of today and education into university worldwide.

The recent discovery of a mysterious aurora around a brown dwarf has left astronomers astounded. This celestial body, known as W1935, is larger than Jupiter and exhibits infrared emissions from methane in its upper atmosphere. What makes this finding even more intriguing is that W1935 lacks a host star to provide energy for such atmospheric phenomena.

Let’s delve into the captivating details:

Brown Dwarfs: These enigmatic objects are larger than gas giant planets but smaller than stars. They form similarly to stars, arising from collapsing clouds of gas and dust. Brown dwarfs are often isolated, just like W1935. Their nickname, “failed stars,” stems from their inability to sustain nuclear fusion like main-sequence stars.

Auroras: On Earth, we witness auroras as the mesmerizing northern and southern lights. These luminous displays occur when charged solar particles interact with molecules in our atmosphere. Auroras are also observed on other planets, such as Jupiter and Saturn, and over active moons like Io and Enceladus. However, W1935’s aurora is baffling because there are no nearby stars to supply charged particles for this phenomenon .

Infrared Clues: The James Webb Space Telescope (JWST) detected the potential aurora over W1935 through infrared emissions from methane. Similar emissions occur on Jupiter and Saturn due to charged particles heating their atmospheres and creating aurorae. Scientists speculate that internal processes within W1935 or interactions with interstellar plasma might be responsible for its mysterious glow. Alternatively, an influx of particles from a nearby active moon could play a role.

This discovery transforms the astrophysics of today, sparking curiosity and wonder across universities worldwide. The universe continues to surprise us with its hidden secrets, inviting us to explore further into the cosmic unknown.

Giant planets orbiting white dwarfs
A white dwarf for astronomers of this planet is the stellar core left behind after a dying star has exhausted its nuclear fuel and expelled its outer layers to form a planetary nebula.

Chinese astronomers may have spotted Pons-Brooks in 1385, and an Italian astronomer may have glimpsed it in 1457.

Comet 12P/Pons–Brooks has been identified as a comet observed in 1385 and in 1457. The 1385 apparition was very favorable and the comet was recorded by the Chinese in Ming Shilu and was also mentioned in some European sources. Brooks is an intermediate-period comet (orbital period around 71 years) comparable to 1P/Halley that boasts a rich history of cosmic exploration. After other of its sightings , the comet's path was adjusted, and astronomers imagination it would return near the sun on May 27, 1954. Using this prediction, Elizabeth Roemer from Lick Observatory found the comet on June 20, 1953, very close to where it was expected to be. It appeared faint at first but then brightened in July, dimmed again by mid-July, and slowly brightened as it neared its closest approach to the sun.

By September 15, it reached a moderate brightness but had another sudden increase in brightness by the 28th. Another brightening occurred in December before the comet behaved as anticipated. Its brightest point was in late April, reaching magnitude 6.

Between 1740 and 2167, the comet's orbit remains quite stable, with minimal influence from planets. Its closest approach to Earth during this time was 0.634 astronomical units (AU) on January 9, 1884, but Earth's gravity didn't significantly affect its path.

Many appearance in 2024 will probably be a chance to see it. However, otherwise may have another opportunity in the summer of 2095, when 12P/Pons-Brooks will reach its perihelion on August 10.

Protoplanetary disks play a crucial role in the formation of planets around young stars
u/tonynetone1 - This is an AI concept portrays inner protoplanetary disk. New measurements by NASA’s James Webb Space Telescope have detected water vapor
This is an AI concept portrays inner protoplanetary disk. New measurements by NASA’s James Webb Space Telescope have detected water vapor
New measurements by NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument) have detected water vapor in the system’s inner disk

Webb is solving mysteries in our solar system, looking beyond to distant AND mysterious structures THIS technology is an international program led by NASA with its partners

Protoplanetary disks play a crucial role in the formation of planets around young stars. These disks are composed of gas and dust particles, and they orbit a central young star. Over time, the material in the disk starts to clump together due to gravitational forces, eventually forming planets and other celestial bodies.

The recent detection of water vapor in the protoplanetary disk of the PDS 70 system is indeed significant for several reasons. The PDS 70 system is located approximately 370 light-years away from Earth, and it has been a focus of study for astronomers using advanced observational techniques.

The presence of water vapor in the terrestrial zone of the protoplanetary disk is noteworthy because this region is considered the prime location for the formation of rocky planets. The terrestrial zone, also known as the habitable zone or Goldilocks zone, is characterized by conditions suitable for the formation of planets with solid surfaces, where water can exist in liquid form. The detection of water vapor in this zone suggests the possibility of water being available during the formation of rocky planets in the PDS 70 system.

Understanding the composition of protoplanetary disks and the presence of key molecules like water vapor provides valuable insights into the conditions that lead to the formation of planetary systems. It contributes to our broader understanding of the processes involved in planetary formation and the potential for habitable environments in other star systems. This kind of research helps astronomers piece together the puzzle of how planetary systems, including our own solar system, come into existence. Water vapor can indeed be present in the atmospheres of exoplanets (planets outside of our solar system).

Detecting water vapor in exoplanet atmospheres is a significant area of research in the field of exoplanet studies. Scientists use various methods to detect the presence of water vapor on distant exoplanets. One commonly used technique is spectroscopy, which involves analyzing the light from the star that passes through the exoplanet's atmosphere. This analysis allows researchers to identify the presence of specific molecules, including water vapor, by looking for characteristic absorption patterns in the spectrum. The discovery of water vapor in an exoplanet's atmosphere can provide valuable insights into the planet's potential habitability. Water is a crucial ingredient for life as we know it, so the presence of water vapor on exoplanets is often considered an essential factor in determining their potential habitability.

However, it is important to note that the detection of water vapor does not directly imply the presence of liquid water or the habitability of an exoplanet. Many other factors, such as the planet's distance from its star, its composition, and the overall environmental conditions, need to be considered to assess whether an exoplanet may have the right conditions to support life. Ongoing research and technological advancements in space telescopes and spectroscopic techniques are continually improving our understanding of exoplanet atmospheres, including the presence of water vapor. With time, we expect to gather more data and learn more about the atmospheres of exoplanets and their potential for hosting water vapor and, possibly, life.

the solar system was originally created by a big bang when the sun lit and threw matter into space. that matter formed the planets that were trapped by the sun's gravity and have been pulled closer to it ever since. the sun like all stars was created by a big bang.
eventually we will move too close to the sun and die from the heat. paying Bob dole trillions of dollars will not change our fate, but colonizing Mars would give us more time.
originally the earth was too far from the sun for life to exist, but gravity moved us closer until we went into the goldilocks zone, where life can exist because it is not too hot or too cold.
the first humans were born in Africa near the equator where it was the warmest during the ice age. because it was still very cold and there was very little sunlight, the first humans would have been white. Mitochondrial Eve included. eventually the ice melted and the earth warmed. those near the equator got the most heat and tanned first. and that is why we have different skin tones.
also, the neanderthals died because they were vegans.

The Earth is flat?
Well why are all the other planets round then???

A question asked MILLIONS of times, with a very simple explanation!

Here is an entire playlist answering this question!

https://www.youtube.com/playlist?list=PLyHwsN1Rg4Io3Aa14g4XM9pyfgasn7gO7

Yes, the biggest part of the Star Trek Universe was communist in the purist form. The United Federation of Planets eliminated money, and all beings within the Federation worked for the greater good. So in theory, there were no lazy people (bullshit). And everyone got everything that they needed. Some planets outside the federation still dealt in money, like the Ferengi, I think the Klingons did too.

In the Movie, the Voyage Home, Kirk mentions that we still used money. A hint that money was eliminated well before the Next Generation. I refuse to think anything made after Voyager as cannon.

DS9 was shit, and the new series with all those leftists in it is all shit. The movies with the alternate timelines in it is all shit.

Psalms 19:1
The heavens declare the glory of God; and the firmament sheweth his handywork.”

https://odysee.com/@scoobyburn:1/Real-Stars-and-Planets:a