The asteroid Hygiea may qualify as a dwarf planet — and it could steal the title of the smallest dwarf planet in the solar system!
Astronomers have captured high-resolution imagery of Hygiea, the fourth largest rock in the Asteroid Belt (opens in new tab). And low and behold, Hygiea is spherical in shape. That's a pretty important dwarf-planet marker, and the only one Hygiea was missing until now.
Asteroids boast a variety of shapes, but the rounded shape of dwarf planets (opens in new tab) shows that they had enough mass for its own gravity to pull it into this round shape. Hygiea already met the other requirements for dwarf-planet classification since it orbits the sun, is not a moon orbiting another planet and has not cleared other objects out of its own orbit.
Video: Asteroid Hygiea May Be Smallest Dwarf Planet in Our Solar System (opens in new tab)
Related: Meet the Solar System's Dwarf Planets (opens in new tab)
So, how big is this potential new member of the dwarf planet family? The team of astronomers, led by researcher Pierre Vernazza of the Laboratoire d'Astrophysique de Marseille in France constrained Hygiea's size, and estimated its diameter is just over 267 miles (430 kilometers). For comparison, Hygiea is less than one-fifth the width of its most famous cousin, Pluto, which has a diameter of about 1,491 miles (2,400 km).
Ceres (opens in new tab) held the title of smallest dwarf planet until now, with a diameter of almost 590 miles (950 km).
Before Hygiea can be officially upgraded to dwarf planet status, the International Astronomical Union (opens in new tab) — the same group of astronomers who were responsible making Pluto a dwarf planet — must review all the evidence and take a vote.
Video: Where is Hygiea in Our Solar System? (opens in new tab)
"Thanks to these images, Hygiea may be reclassified as a dwarf planet, so far the smallest in the solar system," Vernazza said in a statement (opens in new tab) from the European Southern Observatory (ESO), which manages the SPHERE instrument that produced the high-resolution imagery in the study. SPHERE (which stands for Spectro-Polarimetric High-contrast Exoplanet Research) sits atop the Very Large Telescope (opens in new tab) at ESO's Paranal Observatory in Chile.
"Thanks to the VLT and the new generation adaptive-optics instrument SPHERE, we are now imaging main belt asteroids with unprecedented resolution, closing the gap between Earth-based and interplanetary mission observations," Vernazza added.
A study detailing the new findings was published today (Oct. 28) in Nature Astronomy (opens in new tab).
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- Why Isn't Pluto a Planet Anymore? (opens in new tab)