Related Experiment Video
Updated: May 6, 2026

14:22
Activating Molecules, Ions, and Solid Particles with Acoustic Cavitation
Published on: April 12, 2014
14.7K
The trans-neptunian object UB313 is larger than Pluto.
F Bertoldi1, W Altenhoff, A Weiss
1Argelander Institute for Astronomy, University of Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany. bertoldi@astro.uni-bonn.de
Nature
|February 3, 2006
Summary
The distant object 2003 UB313 is the largest known trans-Neptunian object, exceeding Pluto in size. Its high reflectivity suggests a methane-rich icy surface, similar to Pluto.
Area of Science:
- Astronomy and astrophysics
- Planetary science
- Solar System dynamics
Background:
- 2003 UB313, a distant Solar System object, was discovered near aphelion.
- Its orbital characteristics (high eccentricity, inclination) classify it as a 'scattered disk' object.
- Scattered disk objects likely originate from the Kuiper Belt, a region of icy bodies beyond Neptune.
Purpose of the Study:
- To determine the actual size and surface properties of 2003 UB313.
- To compare 2003 UB313 with Pluto and other trans-Neptunian objects.
- To understand the composition and reflectivity of distant Solar System bodies.
Main Methods:
- Observations of thermal emission at a wavelength of 1.2 mm.
- Combined thermal emission data with optical brightness measurements.
- Calculated diameter and albedo based on observed data and accounting for measurement uncertainties and object orientation.
Main Results:
- 2003 UB313 has a diameter of 3,000 +/- 300 +/- 100 km, making it larger than Pluto (2,300 km).
- The object's albedo is 0.60 +/- 0.10 +/- 0.05, indicating a highly reflective surface.
- The albedo is similar to Pluto's, suggesting a methane-induced icy surface composition.
Conclusions:
- 2003 UB313 is the largest known trans-Neptunian object.
- Its surface composition is likely icy and highly reflective, similar to Pluto.
- This finding contributes to our understanding of the diversity and properties of objects in the outer Solar System.
Related Concept Videos
Nuclear Transmutation
13.0K
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed...
13.0K
Enlargement of the Plasma Membrane
1.8K
Cell division and enlargement are processes that require precise control. The control ensures that cell division cannot proceed unless the cell has grown to a specific size. A spherical, dividing cell requires an approximately 1.6X increase in its surface area to double its volume. The secretory pathway also has a significant role in cell membrane enlargement. Secretory vesicles that bud off from the Golgi apparatus and later fuse with the plasma membrane during exocytosis are a major source of...
1.8K
Kepler's First Law of Planetary Motion
4.9K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
4.9K
Kepler's Second Law of Planetary Motion
4.7K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
4.7K
Kepler's Third Law of Planetary Motion
3.6K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
3.6K
Diversity of Protists III
2.1K
Rhizaria are a diverse group of unicellular protists characterized by their threadlike cytoplasmic extensions known as pseudopodia. These structures aid in both locomotion and feeding, giving Rhizaria an amoeboid appearance. Their amoeboid morphology once led to taxonomic confusion, but molecular phylogenetics has clarified their evolutionary placement and emphasized their shared use of pseudopodia despite divergent lineages.This clade comprises diverse lineages such as Chlorarachniophyta,...
2.1K

