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1241 Dysona

Asteroid


Asteroid

FieldValue
minorplanetyes
name1241 Dysona
background#D6D6D6
image1241Dysona (Lightcurve Inversion).png
captionLightcurve-based 3D-model of Dysona
discovery_ref
discovererH. E. Wood
discovery_siteJohannesburg Obs.
discovered4 March 1932
mpc_name(1241) Dysona
alt_names
1945 RA1948 CE
1956 PBA908 DC
A920 EB
named_afterFrank Watson Dyson
(English astronomer)
mp_categorymain-belt(outer)
background
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc97.31 yr (35,542 days)
aphelion3.5165 AU
perihelion2.8633 AU
semimajor3.1899 AU
eccentricity0.1024
period5.70 yr (2,081 days)
mean_anomaly290.13°
mean_motion/ day
inclination23.518°
asc_node322.27°
arg_peri320.07°
dimensionskm
km
km
km
km
km
km
rotationh
8.60738 h
h
albedo
spectral_typeTholen PDC
B–V 0.750
U–B 0.290
abs_magnitude9.459.74

1945 RA1948 CE 1956 PBA908 DC A920 EB (English astronomer) background km km km km km km 8.60738 h h

B–V 0.750 U–B 0.290

1241 Dysona, provisional designation , is a dark background asteroid from the outer regions of the asteroid belt, approximately 77 kilometers in diameter. It was discovered on 4 March 1932, by English astronomer Harry Edwin Wood at the Union Observatory in Johannesburg, South Africa. The asteroid was named after English astronomer Frank Watson Dyson.

Orbit and classification

Dysona is a non-family asteroid from the main belt's background population. It orbits the Sun in the outer main-belt at a distance of 2.9–3.5 AU once every 5 years and 8 months (2,081 days; semi-major axis of 3.19 AU). Its orbit has an eccentricity of 0.10 and an inclination of 24° with respect to the ecliptic.

The asteroid was first observed as at Taunton Observatory (803) in February 1908. The body's observation arc begins with its observations as at Heidelberg Observatory in March 1920, or 12 years prior to its official discovery observation at Johannesburg.

Physical characteristics

In the Tholen classification, Dysonas spectral type is ambiguous, closest to a primitive P-type and somewhat similar to a D- and C-type asteroid (PDC).

Rotation period and pole

In April 2006, a rotational lightcurve of Dysona was obtained by Julian Oey at Leura Observatory (E17) in Australia. Lightcurve analysis gave a rotation period of 8.6080 hours with a brightness variation of 0.24 magnitude (), superseding photometric observations by Jean-Gabriel Bosch and Laurent Brunetto in October 2010, who measured a period of 8.355 hours and an amplitude of 0.25 magnitude ().

In 2016, a modeled lightcurve using data from UAPC, the Palomar Transient Factory survey, and individual observers, gave a concurring period of 8.60738 hours as well an astronomical pole of (125.0°, −68.0°) in ecliptic coordinates (λ, β).

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Dysona measures between 70.757 and 83.05 kilometers in diameter and its surface has an albedo between 0.04 and 0.0585.

The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0425 and a diameter of 83.05 kilometers based on an absolute magnitude of 9.45.

Naming

This minor planet was named after English astronomer Frank Watson Dyson (1868–1939), Astronomer Royal of England, director of the Royal Observatory, Greenwich, awarded the Bruce Medal in 1922, and president of the International Astronomical Union from 1928 to 1932. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 114). The lunar crater Dyson was also named in his honor.

References

Info: Wikipedia Source

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