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— CH. 1 · DISCOVERY AND EARLY HISTORY —

2 Pallas

~4 min read · Ch. 1 of 6
6 sections
  • Heinrich Wilhelm Matthias Olbers spotted a moving object on the night of the 28th of March 1802. This discovery occurred just months after Giuseppe Piazzi found Ceres in 1801. Astronomers initially classified this new body as a planet alongside Ceres and other early finds. The German astronomer named the object Pallas, an epithet for the Greek goddess Athena. Estimates of its size reached as high as 3,380 kilometers in diameter shortly after discovery. By 1979, scientists revised that figure down to 673 kilometers, which remains 26% greater than today's accepted value. The discovery sparked intense interest within the astronomy community regarding gaps between Mars and Jupiter. Carl Friedrich Gauss computed the preliminary orbit for both Ceres and Pallas. Their orbital periods proved similar at approximately 4.6 years each. Charles Messier had actually recorded the object on a star chart during April 1779 but assumed it was merely a star.

  • Pallas orbits with an inclination of 34.8 degrees relative to the ecliptic plane. This angle makes the asteroid unusually accessible compared to most other large solar system bodies. Its orbital eccentricity approaches values seen in Pluto itself. Every Palladian summer or winter lasts roughly two Earth years due to an axial tilt of 84 degrees. Large portions of the surface experience constant sunlight or darkness during these extended seasons. The asteroid passed just 8.5 arcminutes south of Sirius on the 9th of October 2022. No planet can approach closer than 30 degrees to that bright star. Pallas maintains a near-1:1 resonance with Ceres while holding a 5:2 resonance with Jupiter over 83-year cycles. These dynamic parameters create unique conditions for future spacecraft missions attempting flybys.

  • Spectroscopic data reveals a B-type asteroid composition rich in olivine and pyroxene minerals. The surface resembles Renazzo carbonaceous chondrite meteorites discovered in Italy during 1824. This material contains little iron and water compared to similar objects like Ceres. Craters larger than 40 kilometers cover at least 9% of the visible surface area. As of 2020, astronomers identified 36 distinct craters across both hemispheres. Provisional names include Akontia meaning dart and Doru meaning pike. A single bright spot appears in the southern hemisphere resembling salt deposits found elsewhere. Radio signals from Mars orbiters helped estimate mass through tiny gravitational perturbations induced on Mars itself. The object lacks hydrostatic equilibrium due to its current rotational period and shape deviations.

  • Pallas likely represents a surviving remnant protoplanet from early Solar System formation epochs. Most other bodies grew into planets or were ejected by planetary gravity during accretion phases. Only Pallas, Vesta, and Ceres remain intact within Neptune's orbit today. Its interior probably never reached temperatures near 820 Kelvin required for dehydration processes. This suggests a homogeneous composition without differentiated dry silicate cores beneath hydrated mantles. Water migration toward the surface may have created salt deposits explaining high albedo values. One theory posits that near-Earth asteroid 3200 Phaethon originated as an ejected piece of Pallas. Such a connection could explain sodium abundance observed in Geminid meteor showers caused by Phaethon.

  • Astronomers used star occultation events to determine accurate diameter measurements before spacecraft visits. Over 140 observers tracked the best-documented event occurring on the 29th of May 1983. These observations provided the first precise calculation of physical dimensions despite distance constraints. A possible tiny satellite with roughly 1 kilometer diameter appeared after data collected on the 29th of May 1979. That moon claim remained unconfirmed by subsequent studies. The Dawn team secured viewing time on Hubble Space Telescope during September 2007. They sought comparative data against Ceres and Vesta at closest approach points every twenty years. Radio signals from Mars orbiters helped estimate mass through gravitational perturbations induced on Mars itself.

  • No spacecraft has ever visited Pallas directly despite multiple proposals over decades. High orbital inclination prevented flyby opportunities for the Dawn probe visiting nearby asteroids. The Athena SmallSat mission planned launch in 2022 as secondary payload alongside Psyche. Authors described it as the largest unexplored main-belt protoplanet available for study. Funding competition ultimately favored other concepts like TransOrbital Trailblazer Lunar Orbiter instead. Scientists continue seeking ways to reach this distant body given its unique scientific value. Current estimates place volume at approximately 90, 95% that of Vesta while holding 7% total asteroid belt mass. Future missions aim to resolve questions about internal structure and surface history without direct sampling capabilities yet available.

Common questions

When did Heinrich Wilhelm Matthias Olbers discover 2 Pallas?

Heinrich Wilhelm Matthias Olbers discovered 2 Pallas on the night of the 28th of March 1802. This event occurred just months after Giuseppe Piazzi found Ceres in 1801.

What is the current diameter of 2 Pallas compared to early estimates?

Scientists revised the size of 2 Pallas down to 673 kilometers by 1979, which remains 26% greater than today's accepted value. Early estimates reached as high as 3,380 kilometers in diameter shortly after discovery.

How does the orbit of 2 Pallas differ from other large solar system bodies?

Pallas orbits with an inclination of 34.8 degrees relative to the ecliptic plane, making it unusually accessible compared to most other large solar system bodies. Its orbital eccentricity approaches values seen in Pluto itself and it maintains a near-1:1 resonance with Ceres while holding a 5:2 resonance with Jupiter over 83-year cycles.

What minerals make up the surface composition of 2 Pallas?

Spectroscopic data reveals that 2 Pallas has a B-type asteroid composition rich in olivine and pyroxene minerals. The surface resembles Renazzo carbonaceous chondrite meteorites discovered in Italy during 1824 and contains little iron and water compared to similar objects like Ceres.

Has any spacecraft ever visited 2 Pallas directly?

No spacecraft has ever visited 2 Pallas directly despite multiple proposals over decades. High orbital inclination prevented flyby opportunities for the Dawn probe visiting nearby asteroids and funding competition ultimately favored other concepts like TransOrbital Trailblazer Lunar Orbiter instead.