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Is Pluto A Planet Essay Introduction


On August 24, 2006 the IAU stripped Pluto of its status as a planet - instead it is now classified as a "dwarf planet." Read about the details on my Blog.

The Applied Physics Laboratory (one of the lead investigators of the New Horizons project) announced the official names of Pluto's second and third moon: Nix and Hydra. This means Pluto now has three moons. More details below.

Clyde W. Tombaugh, staff member at the Lowell Observatory, discovered Pluto on February 18, 1930. The process was painful, the result of "blinking" where two photographic plates are compared against each other to look for any changes in object appearance and position.

Our knowledge of Pluto comes as a result of mathematic and spectroscopy. We know that Pluto is composed of the same rock-ice material as the moons of Uranus and Neptune. It is likely that Pluto's surface contains a combination of carbon dioxide ice, methane ice, and nitrogen ice.

Pluto - A Quick Summary: (More information available on the Pluto Fact Sheet)

Average Distance from Sun:5.915 x 109 km
Eccentricity of Orbit:0.2501
Average Orbital Speed:4.7 km/s
Orbital Period:248.60 years
Rotational Period:6.387 days
Inclination of Equator to Orbit122.52º
Diameter:2,300 km
Mass:1.3 x 1022 kg
Average Density:1900 kg/m3
Escape Speed:1.2 km/s
Albedo:0.5
Average Surface Temperature:-233º C
Atmospheric Composition:None

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Pluto may have two additional moons, which could make 3 moons for Pluto. Observations using the Hubble Space Telescope in May of 2005 demonstrated two candidates.

More details can be found at the Hubble Space Telescope website.

What is surprising about Pluto is that it has a moon - sort of. The moon of Pluto - called Charon - was discovered in 1978. The composition of Charon is thought to be identical to Pluto.

The current idea is that Charon is not a moon, but a member of the Pluto-Charon system (a binary planet). Charon does not orbit Pluto and Pluto does not orbit Charon. Instead, the both rotate about a common point.

There is also debate as to the planet classification of Pluto:

  • Composition of Pluto and Charon is though to be identical to the Kuiper Belt Objects
  • The inclination of Pluto's orbit is 17º , a secondary signature of a captured body
  • Pluto's orbit brings the planet closer to the Sun than Neptune on during it annual orbit

These issues will hopefully be answered when the New Horizons probe arrives at Pluto.

Nix and Hydra:

The discovery team responsible for the New Horizons project also discovered (its official now) the two additional satellites in May of 2005. What is more remarkable is the tool used to discover the moons: the Hubble Space Telescope. The two new moons are 5000 times more faint than Pluto and two to three times the Pluto-Charon distance.

The team initially names the moons Nyx S/2005 P2 and Hydra S/2005 P1. Nyx was renamed to Nix by the IAU since asteroid 3908 bears the name Nyx (the name of the Greek goddess of darkness and night). Nix is the Egyptian equivalent to Nyx. Hydra is the mythological sea serpent with nine heads.

A bit of trivia: the first two letters of Pluto (P and L) is used to honor Percival Lowell who motivated the search for Pluto. In addition, the first letters of Nix and Hydra are used to honor the New Horizons mission and the Hubble Space Telescope (the letters N and H).

Hydra is the brighter (possibly larger) outer moon while Nix is the  dimmer (possibly smaller) middle moon (Charon is closest to Pluto and the brightest moon). The orbit's of Nix and Hydra are near circular and are on the same plane as Charon - but at greater distance. This demonstrates a possible common origin of Charon, Nix and Hydra - the result of a large impact of some object with Pluto.

Astronomers will point their telescopes toward these two new moons in order to learn their properties. In addition, the arrival of New Horizons in 2015 will provide detailed mapping.

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Pluto, once considered the ninth and most distant planet from the sun, is now the largest known dwarf planet in the solar system. It is also one of the largest known members of the Kuiper Belt, a shadowy zone beyond the orbit of Neptune thought to be populated by hundreds of thousands of rocky, icy bodies each larger than 62 miles (100 kilometers) across, along with 1 trillion or more comets. 

In 2006, Pluto was reclassified as a dwarf planet, a change widely thought of as a demotion. The question of Pluto's planet status has attracted controversy and stirred debate in the scientific community, and among the general public, since then. In 2017, a science group (including members of the New Horizon mission) proposed a new definition of planethood based on "round objects in space smaller than stars," which would make the number of planets in our solar system expand from 8 to roughly 100.

American astronomer Percival Lowell first caught hints of Pluto's existence in 1905 from odd deviations he observed in the orbits of Neptune and Uranus, suggesting that another world's gravity was tugging at these two planets from beyond. Lowell predicted the mystery planet's location in 1915, but died without finding it. Pluto was finally discovered in 1930 by Clyde Tombaugh at the Lowell Observatory, based on predictions by Lowell and other astronomers.

Pluto got its name from 11-year-old Venetia Burney of Oxford, England, who suggested to her grandfather that the new world get its name from the Roman god of the underworld. Her grandfather then passed the name on to Lowell Observatory. The name also honors Percival Lowell, whose initials are the first two letters of Pluto. 

Physical characteristics

Since Pluto is so far from Earth, little was known about the dwarf planet's size or surface conditions until 2015, when NASA's New Horizons space probe made a close flyby of Pluto. New Horizons showed that Pluto has a diameter of 1,473 miles (2,370 km), less than one-fifth the diameter of Earth, and only about two-thirds as wide as Earth's moon.

Observations of Pluto's surface by the New Horizons spacecraft revealed a variety of surface features, including mountains that reach as high as 11,000 feet (3,500 meters), comparable to the Rocky Mountains on Earth. While methane and nitrogen ice cover much of the surface of Pluto, these materials are not strong enough to support such enormous peaks, so scientists suspect that the mountains are formed on a bedrock of water ice. [Photos of Pluto and Its Moons]

Pluto's surface is also covered in an abundance of methane ice, but New Horizons scientists have observed significant differences in the way the ice reflects light across the dwarf planet's surface. The dwarf planet also possesses ice ridge terrain that appears to look like a snakeskin; astronomers spotted similar features to Earth's penitentes, or erosion-formed features on mountainous terrain. The Pluto features are much larger; they are estimated at 1,650 feet (500 m) tall, while the Earth features are only a few meters in size.  

Another distinct feature on Pluto's surface is a large heart-shaped region known unofficially as Tombaugh Regio (after Clyde Tombaugh; regio is Latin for region). The left side of the region (an area that takes on the shape of an ice cream cone) is covered in carbon monoxide ice. Other variations in the composition of surface materials have been identified within the "heart" of Pluto.

In the center left of Tombaugh Regio is a very smooth region unofficially known by the New Horizons team as "Sputnik Planum," after Earth's first artificial satellite, Sputnik. This region of Pluto's surface lacks craters caused by meteorite impacts, suggesting that the area is, on a geologic timescale, very young — no more than 100 million years old. It's possible that this region is still being shaped and changed by geologic processes.

These icy plains also display dark streaks that are a few miles long, and aligned in the same direction. It's possible the lines are created by harsh winds blowing across the dwarf planet's surface.

NASA's Hubble Space Telescope has also revealed evidence that Pluto's crust could contain complex organic molecules.

Pluto's surface is one of the coldest places in the solar system, at roughly minus 375 degrees Fahrenheit (minus 225 degrees Celsius). When compared with past images, pictures of Pluto taken by the Hubble Space Telescope revealed that the dwarf planet had apparently grown redder over time, apparently due to seasonal changes.

Pluto may have (or may have had) a subsurface ocean, although the evidence is still out on that finding. If the subsurface ocean existed, it could have greatly affected Pluto's history. For example, scientists found that the zone of Sputnik Planitia redirected Pluto's orientation due to the amount of ice in the area, which was so heavy it affected Pluto overall; New Horizons estimated the ice is roughly 6 miles (10 km thick). A subsurface ocean is the best explanation for the evidence, the researchers added, although looking at less likely scenarios, a thicker ice layer or movements in the rock may be responsible for the movement. If Pluto did have a liquid ocean, and enough energy, some scientists think Pluto could harbor life.

Orbital characteristics

Pluto's highly elliptical orbit can take it more than 49 times as far out from the sun as Earth. Since the dwarf planet's orbit is so eccentric, or far from circular, Pluto's distance from the sun can vary considerably. The dwarf planet actually gets closer to the sun than Neptune is for 20 years out of Pluto's 248-Earth-years-long orbit, providing astronomers a rare chance to study this small, cold, distant world.

As a result of that orbit, after 20 years as the eighth planet (in order going out from the sun), in 1999, Pluto crossed Neptune's orbit to become the farthest planet from the sun (until it was demoted to the status of dwarf planet).

When Pluto is closer to the sun, its surface ices thaw and temporarily form a thin atmosphere, consisting mostly of nitrogen, with some methane. Pluto's low gravity, which is a little more than one-twentieth that of Earth's, causes this atmosphere to extend much higher in altitude than Earth's. When traveling farther away from the sun, most of Pluto's atmosphere is thought to freeze and all but disappear. Still, in the time that it does have an atmosphere, Pluto can apparently experience strong winds. The atmosphere also has brightness variations that could be explained by gravity waves, or air flowing over mountains. 

While Pluto's atmosphere is too thin to allow liquids to flow today, they may have streamed along the surface in the ancient past. New Horizons imaged a frozen lake in Tombaugh Regio that appeared to have ancient channels nearby. At some point in the ancient past, the planet could have had an atmosphere roughly 40 times thicker than on Mars. 

In 2016, scientists announced that they might have spotted clouds in Pluto's atmosphere using New Horizons data. Investigators saw seven bright features that are near the terminator (the boundary between daylight and darkness), which is commonly where clouds form. The features are all low in altitude and roughly about the same size, indicating that these are separate features. The composition of these clouds, if they are indeed clouds, would likely be acetylene, ethane and hydrogen cyanide. 

Composition & structure

Some of Pluto's parameters, according to NASA:

Atmospheric composition: Methane, nitrogen. Observations by New Horizons show that Pluto's atmosphere extends as far as 1,000 miles (1,600 km) above the surface of the dwarf planet.

Magnetic field: It remains unknown whether Pluto has a magnetic field, but the dwarf planet's small size and slow rotation suggest it has little to no such field.

Chemical composition: Pluto probably consists of a mixture of 70 percent rock and 30 percent water ice.

Internal structure: The dwarf planet probably has a rocky core surrounded by a mantle of water ice, with more exotic ices such as methane, carbon monoxide and nitrogen ice coating the surface.

Orbit & rotation

Pluto's rotation is retrograde compared to the solar systems' other worlds; it spins backward, from east to west.

Average distance from the sun: 3,670,050,000 miles (5,906,380,000 km) — 39.482 times that of Earth

Perihelion (closest approach to the sun): 2,756,902,000 miles (4,436,820,000 km) — 30.171 times that of Earth

Aphelion (farthest distance from the sun): 4,583,190,000 miles (7,375,930,000 km) — 48.481 times that of Earth

Pluto's moons

Pluto has five moons: Charon, Styx, Nix, Kerberos and Hydra, with Charon being the closest to Pluto and Hydra the most distant.

In 1978, astronomers discovered that Pluto had a very large moon nearly half the dwarf planet's own size. This moon was dubbed Charon, after the mythological demon who ferried souls to the underworld in Greek mythology.

Because Charon and Pluto are so similar in size, their orbit is unlike that of most planets and their moons. Both Pluto and Charon orbit a point in space that lies between them, similar to the orbits of binary star systems, For this reason, scientists refer to Pluto and Charon as a double dwarf planet, double planet or binary system.

Pluto and Charon are just 12,200 miles (19,640 km) apart, less than the distance by flight between London and Sydney. Charon's orbit around Pluto takes 6.4 Earth-days, and one Pluto rotation — a Pluto-day — also takes 6.4 Earth-days. This is because Charon hovers over the same spot on Pluto's surface, and the same side of Charon always faces Pluto, a phenomenon known as tidal locking.

While Pluto has a reddish tint, Charon appears more grayish. In its early days, the moon may have contained a subsurface ocean, though the satellite probably can't support one today.

Compared with most of the solar system's planets and moons, the Pluto-Charon system is tipped on its side in relation to the sun.

Observations of Charon by New Horizons have revealed the presence of canyons on the moon's surface. The deepest of those canyons plunges downward for 6 miles (9.7 km). A long swatch of cliffs and troughs stretches for 600 miles (970 km) across the middle of the satellite. A section of the moon's surface near one pole is covered in a much darker material than the rest of the planet. Similar to regions of Pluto, much of Charon's surface is free of craters — suggesting the surface is quite young and geologically active. Scientists saw evidence of landslides on its surface, the first time such features have been spotted in the Kuiper Belt. The moon may have also possessed its own version of plate tectonics, which cause geologic change on Earth. 

In 2005, scientists photographed Pluto with the Hubble Space Telescope in preparation for the New Horizons mission and discovered two other tiny moons of Pluto, now dubbed Nix and Hydra. These satellites are two and three times farther away from Pluto than is Charon. Based on measurements by New Horizons, Nix is estimated to be 26 miles (42 km) long and 22 miles (36 km) wide, while Hydra is estimated at 34 miles (55 km) long and 25 miles (40 km) wide. It is likely that Hydra's surface is coated primarily in water ice.

Scientists using Hubble discovered a fourth moon, Kerberos, in 2011. This moon is estimated to be 8 to 21 miles (13 to 34 km) in diameter. On July 11, 2012, a fifth moon, Styx, was discovered (with an estimated width of 6 miles or 10 km), further fueling the debate about Pluto's status as a planet.

The four newly spotted moons may have formed from the collision that created Charon. Their orbits have been found to be highly chaotic.

Research & exploration

NASA's New Horizons mission is the first probe to study Pluto, its moons and other worlds within the Kuiper Belt up close. It was launched on January 2006, and successfully made its closest approach to Pluto on July 14, 2015. The last of the data was downloaded to Earth in 2016. New Horizons is now on its way to the Kuiper Belt object 2014 MU69, which it will fly by on Jan. 1, 2019. 

The New Horizons probe carries some of the ashes of Pluto's discoverer, Clyde Tombaugh.

The limited knowledge of the Pluto system created unprecedented dangers for the New Horizons probe. Prior to the mission's launch, scientists knew of the existence of only three moons around Pluto. The discovery of Kerberos and Styx during the spacecraft's journey fueled the idea that more satellites could orbit the dwarf planet, unseen from Earth. Collisions with unseen moons, or even small bits of debris, could have seriously damaged the spacecraft. But the New Horizons design team equipped the space probe with tools to protect it during its journey.

Pluto's formation & origins

The leading hypothesis for the formation of Pluto and Charon is that a nascent Pluto was struck with a glancing blow by another Pluto-size object. Most of the combined matter became Pluto, while the rest spun off to become Charon, this idea suggests. [Infographic: Pluto: A Dwarf Planet Oddity]

Additional reporting by staff writer Calla Cofield and by Elizabeth Howell and Nola Taylor Redd, Space.com contributors.

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