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Pluto

Pluto was discovered in 1930 by Clyde Tombaugh, a young American astronomer working in Arizona. The search for Pluto, began much earlier, in the early 20th century, due to observations of small irregularities in the orbits of Uranus and Neptune. These anomalies suggested the presence of a "Planet X," a large, unseen planet exerting a gravitational influence.


Percival Lowell, an influential American astronomer, initiated the search for this mysterious planet. He dedicated years of effort to the project, laying the foundation for Clyde Tombaugh’s eventual discovery, although Lowell passed away before seeing the results of his work. Later calculations revealed that the observed irregularities were due to observational errors, not the gravitational pull of another planet. Nevertheless, Tombaugh’s discovery of Pluto was a monumental achievement, representing a blend of meticulous observation and technological advancement.


Photo of Pluto -NASA

Pluto's Location and It's Geological Activity

Pluto is located in the Kuiper Belt. With a diameter of about 2,377 kilometers, it’s smaller than Earth's Moon and even smaller than some other moons in solar system, such as Ganymede and Titan. Despite its size, Pluto has a surprisingly diverse surface. Images from NASA’s New Horizons Mission in 2015 revealed vast icy plains, towering mountains made of water ice, and even possible cryovolcanoes that may erupt with slushy mixtures of water and other materials. These discoveries highlighted Pluto's geological activity and showed that it is far from being just a frozen, inert world.


The Beginning of The Main Part of The Kuiper Belt- NASA

Tombaugh Regio and Pluto's Atmosphere

One of the most fascinating features on Pluto is the heart-shaped region called Tombaugh Regio, named in honor of its discoverer. This region includes a vast plain known as Sputnik Planitia, which is composed of nitrogen ice. Scientists believe this icy plain is constantly renewing itself through convection, making it one of the youngest surfaces in the solar system. This dynamic surface challenges science environment’s understanding of geological processes and proves that even distant celestial bodies can harbor active landscapes. 


Pluto’s atmosphere is another intriguing feature. Although thin, it is primarily composed of nitrogen, with traces of methane and carbon monoxide. What’s fascinating is that this atmosphere expands when Pluto is closer to the Sun in its highly elliptical orbit and freezes back onto the surface when it moves farther away. This seasonal behavior is unique and highlights the complexity of even a small celestial body such as Pluto. 


A color map of Pluto's surface with a combination of formal and informal feature names indicated.-The Astronomical Journal

The Debate on Pluto's Status

In 2006, the International Astronomical Union introduced a new definition of what constitutes a planet. According to this definition, a celestial body must orbit the Sun, have enough mass to be nearly spherical, and clear its orbit of other debris. While Pluto meets the first two criteria, it does not meet the third because it shares its orbital space with other objects in the Kuiper Belt. This is why it was reclassified as a "dwarf planet," a decision that sparked both scientific debate and public outcry.


The reclassification of Pluto is a poignant example of how science evolves. The decision was not about diminishing Pluto’s importance but rather about refining our understanding of the solar system. This shift allowed astronomers to explore the Kuiper Belt in greater detail, leading to the discovery of other intriguing dwarf planets such as Eris, Haumea, and Makemake. The Kuiper Belt is now recognized as a dynamic region full of scientific potential, offering insights into the early solar system's formation and evolution.

The public’s emotional attachment to Pluto is undeniable. Many people grew up learning about Pluto as the ninth planet, and its demotion felt like losing a member of the solar system family. Some even campaigned to restore Pluto's planetary status. While the controversy continues, the discussion has sparked greater public interest in astronomy and planetary science, demonstrating how debates in science can engage and educate the public. 


People gather on the New Mexico State University campus to protest Pluto's loss of status as a planet in 2006. (New Mexico State University)-CBC News

Life Potential on Pluto

Despite its new status, Pluto remains an essential object of study. NASA’s New Horizons mission, which flew by Pluto in 2015, provided incredible data. It showed people that even small celestial bodies can be complex and dynamic. For example, scientists believe there could be a liquid water ocean beneath Pluto's icy surface, raising the possibility that it could harbor life—or at least conditions for life. This discovery makes Pluto a key target in the search for understanding the potential habitability of other worlds. 


To conclude, Pluto’s story is not just about losing its planet status. It’s about how science adapts and evolves with new discoveries. From its discovery in 1930 to the revelations of the New Horizons mission, Pluto continues to surprise and inspire humanity. Its journey from "Planet X" to a dwarf planet highlights the ever-changing nature of science and reminds people that even a small, icy world at the edge of the solar system can have a profound impact on their understanding of the universe. Whether people call it a planet or a dwarf planet, Pluto remains a symbol of exploration, curiosity, and the boundless potential of scientific discovery.

Bibliographies

CBC News. “Pluto Scientists Battle Planet Definition.” CBC, 2017. https://www.cbc.ca/news/science/pluto-scientists-battle-planet-definition-1.4032382.


Bottke, W. F., et al. “The Origin of Asteroids and the Kuiper Belt.” Earth and Planetary Science Letters 455 (2016): 1-12. https://www.sciencedirect.com/science/article/abs/pii/S0019103516305267.

Gordon, K. D., et al. “The Search for Kuiper Belt Objects.” The Astronomical Journal 153, no. 5 (2017): 1-10. https://iopscience.iop.org/article/10.3847/1538-3881/aa965b/meta.


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Main AuthorSude Nur AkgülFebruary 9, 2025 at 6:10 PM
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