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9994 Grotius

Rafita asteroid


Rafita asteroid

FieldValue
minorplanetyes
name9994 Grotius
background#D6D6D6
imageAnimatedOrbitOf9994Grotius.gif
caption
discovery_ref
discovered24 September 1960
discovererC. J. van Houten
I. van Houten-G.
T. Gehrels
discovery_sitePalomar Obs.
mpc_name(9994) Grotius
alt_names4028 P-L
pronounced
named_afterHugo Grotius
(Dutch jurist)
mp_categorymain-belt(middle)
Rafita
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc55.59 yr (20,306 days)
aphelion3.0391 AU
perihelion2.1307 AU
semimajor2.5849 AU
eccentricity0.1757
period4.16 yr (1,518 days)
mean_anomaly204.01°
mean_motion/ day
inclination7.1806°
asc_node207.15°
arg_peri224.33°
dimensions3.38 km (calculated)
km
rotationh
albedo0.20 (assumed)
spectral_typeS
abs_magnitude14.2 (R)14.314.72

I. van Houten-G. T. Gehrels (Dutch jurist) Rafita km

9994 Grotius , provisional designation , is a stony Rafita asteroid from the middle regions of the asteroid belt, approximately 3.5 kilometers in diameter. It was discovered during the Palomar–Leiden survey in 1960, and named after Dutch jurist Hugo Grotius.

Discovery

Grotius was discovered on 24 September 1960, by the Dutch astronomers Ingrid and Cornelis van Houten, on photographic plates taken by Dutch–American astronomer Tom Gehrels at Palomar Observatory in California, United States.

Survey designation

The survey designation "P-L" stands for Palomar–Leiden, named after Palomar Observatory and Leiden Observatory, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.

Orbit and classification

Grotius orbits the Sun in the central main-belt at a distance of 2.1–3.0 AU once every 4 years and 2 months (1,518 days). Its orbit has an eccentricity of 0.18 and an inclination of 7° with respect to the ecliptic. The body's observation arc begins with its official discovery observation at Palomar.

Rotation period

In August 2010, a rotational lightcurve of Grotius was obtained from photometric observations in the R-band at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 9.2189 hours with a brightness variation of 0.27 magnitude ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Grotius measures 3.746 kilometers in diameter and its surface has an albedo of 0.263. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.38 kilometers based on an absolute magnitude of 14.72.

Naming

This minor planet was named for Dutch jurist Hugo Grotius (1583–1645), who laid the foundations for international law, based on natural law. He was a child prodigy and entered Leiden University when he was just eleven years old. The approved naming citation was published by the Minor Planet Center on 11 November 2000 (M.P.C. 41571).

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
Info: Wikipedia Source

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