Astronoo - Back to homepage
X (new window) Bluesky (new window) Pinterest (new window)
English Français Español Português 日本語 Deutsch 中文
Last updated: July 26, 2026

Asteroid Juno: An Underestimated Giant of the Solar System

Asteroid Juno

The artist's representation in the image shows a huge impact crater.
Image source: David A. Aguilar, Harvard-Smithsonian Center for Astrophysics.

Scientific Summary

Juno (3 Juno), discovered in 1804 by Karl Harding, is one of the largest S-type asteroids in the main belt. Its irregular dimensions of 320 × 267 × 200 km (mean diameter ~234 km) reveal a massive body composed of silicates and metals, representative of the rocky materials of the protoplanetary disk. Juno's surface is marked by a huge impact crater, probably resulting from a violent collision. Through its composition, size and traces of visible cataclysmic events, Juno constitutes a fossil of the primitive Solar System. It illuminates the diversity of materials present in the protoplanetary disk and the processes that prevented the formation of a planet between Mars and Jupiter, a region disturbed by the gravity of the latter.

What is asteroid Juno and what is its scientific importance in the main belt?

Juno, officially designated 3 Juno, is the third asteroid discovered (1804) and one of the largest in the main belt, with an average diameter of about 234 km and irregular dimensions of 320 × 267 × 200 km. Astronoo's article presents it as an "underestimated giant", whose study is crucial for several reasons. Firstly, its S-type classification indicates a composition of silicates and metals, making it a witness to the diversity of materials present in the protoplanetary disk. Secondly, Juno has a remarkable feature: a huge impact crater, probably caused by a collision with another body. The study of this structure, although its exact dimensions remain to be specified, offers a window into the violent collision history that shaped not only asteroids but also planets. Finally, its rapid rotation (7.2 hours) and its orbit (2.67 AU, period of 4.36 years) make it a dynamically interesting object. The article emphasizes that Juno, like other large listed asteroids (Ceres, Pallas, Vesta), is a fossil of the formation of the Solar System, because the main belt represents a region where planet formation was prevented by Jupiter's gravitational perturbations.

Also worth exploring

Continue your exploration of the Universe with these topics:

Asteroid Juno: a large asteroid

Juno, officially designated 3 Juno, is one of the largest asteroids in the main belt. Discovered in 1804 by German astronomer Karl Harding, Juno is the third asteroid to have been identified, after Ceres and Pallas.

Orbit and rotation

Asteroid Juno orbits the Sun at an average distance of 2.67 astronomical units, with an orbital period of about 4.36 Earth years. Its rotation is rapid, with a period of only 7.2 hours, which is relatively short for an asteroid of this size.

Scientific importance

Juno is of great interest to astronomers due to its composition and size. Studies of this asteroid can provide valuable information on the formation and evolution of the solar system. In addition, its surface shows signs of impact craters, which can help understand the collision history in the asteroid belt.

Table of the largest asteroids

The 25 largest asteroids in the main belt
RankNameNumberMean diameterSpectral typeYear of discovery
1Ceres1940 kmC (dwarf planet)1801
2Vesta4525 kmV1807
3Pallas2512 kmB1802
4Hygiea10430 kmC1849
5Interamnia704326 kmF1910
6Europa52315 kmC1858
7Davida511289 kmC1903
8Sylvia87286 kmX1866
9Hektor624250 kmD (Jovian Trojan)1907
10Euphrosyne31248 kmC1854
11Juno3240 kmS1804
12Psyche16226 kmM1852
13Cybele65222 kmX1861
14Thisbe88218 kmB1852
15Camilla107215 kmC1868
16Herculina532212 kmS1872
17Doris48210 kmC1857
18Iris7200 kmS1847
19Patientia451198 kmC1899
20Amphitrite29195 kmS1854
21Lutetia21190 kmM1852
22Bamberga324185 kmC1892
23Egeria13180 kmG1850
24Electra130178 kmG1873
25Eunomia15175 kmS1851

References

FAQ: Everything you need to know about asteroid Juno (3 Juno)

What is asteroid Juno and when was it discovered?

Juno, officially designated 3 Juno, is a large main-belt asteroid. It was discovered in 1804 by German astronomer Karl Harding, making it the third asteroid identified in history, after Ceres (1801) and Pallas (1802).

What are the main physical characteristics of Juno?

Juno is an S-type asteroid, composed primarily of silicates and metals. Its shape is irregular with dimensions of about 320 × 267 × 200 kilometers (mean diameter 234 km). Its rotation period is very rapid, about 7.2 hours, and it orbits the Sun at an average distance of 2.67 astronomical units (AU), with an orbital period of 4.36 Earth years.

Why is Juno a scientifically important object?

Juno is important for several reasons:

What is known about the large crater on Juno?

The article mentions the presence of a huge impact crater on Juno's surface, the result of a violent collision with another body. Although the exact dimensions of the crater are not precisely known, it could cover a significant portion of the surface. Its analysis, via telescope data, makes it possible to estimate the energy of the impact and study the asteroid's internal structure.

What is Juno's position in the main asteroid belt?

Juno is located in the main belt, a region situated between the orbits of Mars and Jupiter (between 300 and 600 million kilometers from the Sun). This zone contains several hundred thousand objects, which could not form a planet because of Jupiter's gravitational perturbations. Juno is one of the largest members of this belt.

Where does Juno rank in terms of size among the largest asteroids?

According to the table provided in the article, Juno (3 Juno) is the 12th largest asteroid on the list presented, with dimensions of 320 × 267 × 200 km. It is preceded by giants like Ceres (974.6 km), Pallas, Vesta, Hygiea, and others, but remains a major object in the main belt.

🏠

To explore in this category

Dwarf Planets: The Forgotten Worlds of the Solar System
Kuiper Belt: Composition and Origins
Haumea and its Moons: A Singularity of the Solar System
The Enigma of the Oort Cloud: Indirect Evidence and Uncertainties
Sedna: The Mysterious Remnant at the Edge of the Solar System
Quaoar: The Dwarf Planet That Defies the Roche Limit with Its Two Rings
What is Dust? Between the Dust on Our Shelves and the Dust that Builds Planets
Ceres: Boundary Between Asteroid and Dwarf Planet
Pluto and its Moons: Charon, Nix, Hydra, Styx, and Kerberos
Eris: The Dwarf Planet at the Edge of the Solar System
Gonggong: An Eccentric Witness to Distant Perturbations
Meteor Showers: Perseids, Leonids, Geminids...
Interstellar Comets: When the Universe Sends its Messengers
The Asteroid Bennu: The Building Blocks of Life
Formation of Asteroids: From Cosmic Dust to Small Rocky Bodies
Yarkovsky Effect: Orbit and Rotation of Asteroids
Arrokoth: Unique Witness to the Primordial Solar Nebula
The Kirkwood Gaps in the Main Asteroid Belt
Asteroid Belt: Dark, Bright, or Red
The Great Comet of 1577 Shattered the Crystal Spheres
The Invisible Threat of Asteroids: From Pebbles to Flying Mountains
Meteorites: Messengers from Space and Witnesses of the Solar System
Comet Hartley 2: The Icy Heart Scrutinized by Deep Impact
When Two Asteroids Collide: The Strange Case of P/2010 A2
2005 YU55: The 400 m Asteroid that Grazed Earth
Asteroid Apophis: The Perfect Candidate for a Global Impact?
Vesta: The Colossus of the Asteroid Belt
From Asteroids to Planets
Comet Ison C/2012: between the promise of brilliance and disillusionment
Giants of the Asteroid Belt: Classification by Size
Impact Craters on Earth: Between Destruction and Mineral Resources
Online Simulator: Orbits of Asteroids
Online Simulator: Orbits of Near-Earth Asteroids
Rosetta has a date with a comet
Near-Earth Asteroids: An Underestimated Threat?
Asteroid 2009 DD45: A Reminder of Planetary Vulnerability to Asteroids
Strange Resemblance Between Comet Hartley 2 and Asteroid Itokawa
Earth Trojan Asteroids: The Companions Sharing our Orbit
Torino Scale: a classification system for impact risks
The Nice Model: Towards an Explanation of the Late Heavy Bombardment
NEO Monitoring: The Case of Asteroid 2012 LZ1
Comet Lemmon C/2012 F6: The green visitor of the southern hemisphere
Asteroid 2012 DA14 passed on February 15, 2013
Near-Earth Asteroid 2012 BX34: A Record Close Approach to Our Planet
Didymos and Dimorphos: The First Asteroid Moon Moved by Humanity
Chariklo and its rings: a surprising centaur asteroid
Rosetta and Philae: A Feat 500 Million Kilometers from Earth
The Passage of Comets: Eccentric Orbits at the Heart of the Solar System
Vesta and its Curiosities: The Enigma of the Torn South Pole
Near-Earth Asteroids: Mapping Celestial Threats
Meeting the Asteroids: The Main Belt
Orbits of Near-Earth Asteroids: When Asteroids Brush Past Earth
Comets: Streaks of Light, Promises of Life, and Cosmic Threats
Asteroid Pallas: A Giant of the Main Belt
Asteroid Juno: an unknown giant of the solar system
Ganymed (1036): Near-Earth and Mars-crosser
Earth's quasi-satellite: 2016 HO3