Pluto was first discovered in 1930 by Clyde W. Tombaugh at the Lowell Observatory in Flagstaff Arizona. Astronomers had long predicted that there would be a ninth planet in the Solar System, which they called Planet X. Only 22 at the time, Tombaugh was given the laborious task of comparing photographic plates. These were two images of a region of the sky, taken two weeks apart. Any moving object, like an asteroid, comet or planet, would appear to jump from one photograph to the next.
After a year of observations, Tombaugh finally discovered an object in the right orbit, and declared that he had discovered Planet X. Because they had discovered it, the Lowell team were allowed to name it. They settled on Pluto, a name suggested by an 11-year old school girl in Oxford, England (no, it wasn’t named after the Disney character, but the Roman god of the underworld).
The Solar System now had 9 planets.
Astronomers weren’t sure about Pluto’s mass until the discovery of its largest Moon, Charon, in 1978. And by knowing its mass (0.0021 Earths), they could more accurately gauge its size. The most accurate measurement currently gives the size of Pluto at 2,400 km (1,500 miles) across. Although this is small, Mercury is only 4,880 km (3,032 miles) across. Pluto is tiny, but it was considered larger than anything else past the orbit of Neptune.
Over the last few decades, powerful new ground and space-based observatories have completely changed previous understanding of the outer Solar System. Instead of being the only planet in its region, like the rest of the Solar System, Pluto and its moons are now known to be just a large example of a collection of objects called the Kuiper Belt. This region extends from the orbit of Neptune out to 55 astronomical units (55 times the distance of the Earth to the Sun).
Astronomers estimate that there are at least 70,000 icy objects, with the same composition as Pluto, that measure 100 km across or more in the Kuiper Belt. And according to the new rules, Pluto is not a planet. It’s just another Kuiper Belt object.
Here’s the problem. Astronomers had been turning up larger and larger objects in the Kuiper Belt. 2005 FY9, discovered by Caltech astronomer Mike Brown and his team is only a little smaller than Pluto. And there are several other Kuiper Belt objects in that same classification.
Astronomers realized that it was only a matter of time before an object larger than Pluto was discovered in the Kuiper Belt.
And in 2005, Mike Brown and his team dropped the bombshell. They had discovered an object, further out than the orbit of Pluto that was probably the same size, or even larger. Officially named 2003 UB313, the object was later designated as Eris. Since its discovery, astronomers have determined that Eris’ size is approximately 2,600 km (1,600 miles) across. It also has approximately 25% more mass than Pluto.
With Eris being larger, made of the same ice/rock mixture, and more massive than Pluto, the concept that we have nine planets in the Solar System began to fall apart. What is Eris, planet or Kuiper Belt Object; what is Pluto, for that matter? Astronomers decided they would make a final decision about the definition of a planet at the XXVIth General Assembly of the International Astronomical Union, which was held from August 14 to August 25, 2006 in Prague, Czech Republic.
Astronomers from the association were given the opportunity to vote on the definition of planets. One version of the definition would have actually boosted the number of planets to 12; Pluto was still a planet, and so were Eris and even Ceres, which had been thought of as the largest asteroid. A different proposal kept the total at 9, defining the planets as just the familiar ones we know without any scientific rationale, and a third would drop the number of planets down to 8, and Pluto would be out of the planet club. But, then… what is Pluto?
In the end, astronomers voted for the controversial decision of demoting Pluto (and Eris) down to the newly created classification of “dwarf planet”.
Is Pluto a planet? Does it qualify? For an object to be a planet, it needs to meet these three requirements defined by the IAU:
- It needs to be in orbit around the Sun – Yes, so maybe Pluto is a planet.
- It needs to have enough gravity to pull itself into a spherical shape – Pluto…check
- It needs to have “cleared the neighborhood” of its orbit – Uh oh. Here’s the rule breaker. According to this, Pluto is not a planet.
What does “cleared its neighborhood” mean? As planets form, they become the dominant gravitational body in their orbit in the Solar System. As they interact with other, smaller objects, they either consume them, or sling them away with their gravity. Pluto is only 0.07 times the mass of the other objects in its orbit. The Earth, in comparison, has 1.7 million times the mass of the other objects in its orbit.
Any object that doesn’t meet this 3rd criteria is considered a dwarf planet. And so, Pluto is a dwarf planet. There are still many objects with similar size and mass to Pluto jostling around in its orbit. And until Pluto crashes into many of them and gains mass, it will remain a dwarf planet. Eris suffers from the same problem.
It’s not impossible to imagine a future, though, where astronomers discover a large enough object in the distant Solar System that could qualify for planethood status. Then our Solar System would have 9 planets again.
Even though Pluto is a dwarf planet, and no longer officially a planet, it’ll still be a fascinating target for study. And that’s why NASA has sent their New Horizons spacecraft off to visit it. New Horizons will reach Pluto in July 2015, and capture the first close-up images of the (dwarf) planet’s surface.
Space enthusiasts will marvel at the beauty and remoteness of Pluto, and the painful deplaneting memories will fade. We’ll just be able to appreciate it as Pluto, and not worry how to categorize it. At least now you know why Pluto was demoted.
If you’d like more information about Pluto. we did two podcasts on this topic at Astronomy Cast. The first discusses the IAU’s decision, and the second is about Pluto and the Icy Outer Solar System. Check them out.
Fakta Baru : Pluto Bukan Planet tapi Planet Kecil
Posted on August 28, 2006 by yOGA
Sidang Umum Himpunan Astronomi Internasional ke-26 mengeluarkan keputusan tentang definisi planet. Ada 3 syarat agar bisa disebut sebagai planet : (a) mengorbit ke matahari, (b) berukuran cukup besar sehingga mampu mempertahankan bentuk (hampir) bulat, dan (c) bersih tidak ada benda langit lain di orbitnya (dikutip dari blog LiveScience : Pluto Poised for Demotion: Details of Thursday’s Vote.
Pluto Bukan Planet
Orbit Pluto memotong orbit Neptunus sehingga Pluto kadang berada lebih dekat dengan Matahari dibanding Neptunus dalam perjalanannya mengelilingi matahari. Hal ini lah yang menyebabkan Pluto harus melepaskan predikatnya sebagai sebuah planet dan mulai sekarang (kecuali ada keputusan baru lagi) termasuk dalam golongan planet kecil (dwarf planet).
Planet Kecil or Dwarf Planets
Syaratnya adalah jika (a) mengorbit ke matahari, (b) berukuran cukup besar sehingga mampu mempertahankan bentuk (hampir) bulat, (c) tidak bersih ada benda langit lain di orbitnya, dan (d) bukan sebuah satelit (ngutip dari blog yang sama).
Sosialisasi
Pemahaman yang kuat bahwa Pluto sebagai sebuah planet sejak diketemukannya di 18 februari 1930 oleh Clyde Tombaugh tentu tidak bisa dengan mudah dihilangkan. Sehingga hal ini menjadi tanggung jawab kita semua untuk ikut mensosialisasikan definisi baru ini. Konsekuensi dari keputusan itu adalah revisi di setiap penyajian informasi yang menyebutkan Pluto sebagai planet, seperti di buku teks, ensiklopedia, kamu termasuk media online spt Wiki….
Hikmah
Perubahan atau aq lebih suka menyebutnya sebagai suatu Revisi seperti ini adalah menjadi konsekuensi dari perkembangan ilmu pengetahuan. Ilmu pengetahuan yang kita ketahui dan kita yakini sekarang bukanlah suatu kesimpulan akhir. Masih banyah hal yang belum kita tahu kebenarannya. Seperti istilah dalam X-Files : the truth is out there
PRAHA, JUMAAT - Ribuan astronomI yang berkumpul di Praha, Ceko akhirnya memutuskan bahwa Pluto tidak termasuk dalam kategori planet pada pertemuan International Astronomical Union (IAU) Kamis (24/8). Alasannya, Pluto tidak memiliki orbit yang dominan seperti lapan planet yang lain. Meskipun demikian, benda langit yang dikenal sebagai planet kesembilan selama 76 tahun di sistem suria dimasukkan ke dalam klasifikasi baru yang disebut planet kerdil. Selain Pluto, Charon, Xena, dan Ceres juga dimasukkan dalam kategori baru ini. "Saya sangat terharu hari ini sebab pada hari terakhir kami harus mendeskripsikan sistem suria sebagaimana mestinya, suka atau tidak," kata Profesor Iwan Williams, ketua panel IAU yang bekerja dalam beberapa bulan terakhir untuk mendefinisikan istilah planet. Definisi yang tegas diperlukan sejak teleskop berteknologi terkini berhasil menunjukkan objek-objek langit baru yang berukuran sebanding Pluto. Tanpa batasan yang tegas, jumlah benda-benda langit yang disebut planet di sistem suria mungkin boleh mencapai 50 atau lebih. Dalam sidang umum IAU, para astronomi sepakat bahwa benda langit dapat disebut sebagai planet jika mengorbit bintang namun bukan sebagai bintang yang memancarkan sinar. Selain itu, ukurannya harus cukup besar sehingga memiliki graviti yang membuatnya berbentuk bulat dan memiliki orbit yang jelas berbeza dengan objek langit lainnya. Pluto secara otomatik tidak memenuhi syarat ini karena orbitnya yang berbentuk elips tumpang tindih dengan orbit Neptun. Orbitnya terhadap Matahari juga terlalu melengkung dibandingkan lapan objek yang diklasifikasikan sebagai planet. Dengan keputusan yang akan ditetapkan IAU ini, definisi mengenai planet-planet di buku teks maupun ensiklopedia harus kemaskini. sistem suria dengan Matahari sebagai pusatnya akan dideskripsikan dengan lapan planet saja. Sementara benda-benda langit lainnya diklasifikasikan tersendiri. Sumber: BBC
Comments
Semoga saya bisa dapat beasiswa ke luar negeri agar kemudian dapat belajar astronomi di negara maju