Skip to content
Surf Wiki
Save to docs
general/rafita-asteroids

From Surf Wiki (app.surf) — the open knowledge base

1658 Innes

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name1658 Innes
background#D6D6D6
discovery_ref
discovered13 July 1953
discovererJ. A. Bruwer
discovery_siteJohannesburg Obs.
mpc_name(1658) Innes
alt_names1953 NA1940 GB
1948 EM1949 QA
1953 OF1953 PN
1957 OE
named_afterRobert T. A. Innes
(astronomer)
mp_categorymain-belt(middle)
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc77.08 yr (28,155 days)
aphelion3.0302 AU
perihelion2.0866 AU
semimajor2.5584 AU
eccentricity0.1844
period4.09 yr (1,495 days)
mean_anomaly247.27°
mean_motion/ day
inclination9.0941°
asc_node95.441°
arg_peri188.76°
dimensionskm
km
km
14.76 km (calculated)
rotationh
albedo0.20 (assumed)
spectral_typeB–V = 0.960
U–B = 0.610
Tholen = ASAS
abs_magnitude10.4711.52

1948 EM1949 QA 1953 OF1953 PN 1957 OE (astronomer) km km 14.76 km (calculated)

U–B = 0.610 Tholen = ASAS

1658 Innes, provisional designation , is a rare-type asteroid from the middle region of the asteroid belt, approximately 15 kilometers in diameter. It was named after Robert T. A. Innes.

Discovery

Innes was discovered on 13 July 1953, by South African astronomer Jacobus Bruwer at Johannesburg Observatory in South Africa.

It was the first numbered discovery of astronomer Jacobus Bruwer. In addition, he also discovered the minor planets 1660 Wood, 1794 Finsen, and 3284 Niebuhr. The asteroid 1811 Bruwer was named in his honour by the Dutch, Dutch-American astronomer trio of the Palomar–Leiden survey.

Orbit and classification

It orbits the Sun in the central main-belt at a distance of 2.1–3.0 AU once every 4 years and 1 month (1,495 days). Its orbit has an eccentricity of 0.18 and an inclination of 9° with respect to the ecliptic. Innes was first identified as at Turku Observatory in 1940, extending the body's observation arc by 13 years prior to its official discovery observation.

Physical characteristics

In the Tholen taxonomy, Innes has an AS-spectral type, an intermediate form of the rare A-types to the common stony asteroids (also see category listing).

Rotation period

In May 2005, astronomers Robert Stephens at the Center for Solar System Studies, California, and Lorenzo Franco at Balzaretto Observatory, near Rome, each obtained a rotational lightcurve of Innes. The photometric observations gave an identical rotation period of hours with a brightness variation of 0.22 and 0.25 magnitude, respectively ().

Diameter and albedo

According to the 2014-revised survey result of NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Innes measures 13.35 kilometers in diameter and its surface has an albedo of 0.248, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 14.76 kilometers with an absolute magnitude of 11.52.

Naming

This minor planet was named for Scottish–South African astronomer Robert T. A. Innes (1861–1933), first director of the discovering Union Observatory from 1903 to 1927 (originally named Transvaal Observatory). He was a skilled observational astronomer, famous for his deliberate search for and discovery of the nearest star, Proxima Centauri, in 1915. He also made important theoretical and computational contributions to celestial mechanics and to the irregular rotation of the Earth. The astronomer is also honored by the lunar crater Innes. The official was published by the Minor Planet Center on 1 July 1972 (M.P.C. 3297).

References

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

Want to explore this topic further?

Ask Mako anything about 1658 Innes — get instant answers, deeper analysis, and related topics.

Research with Mako

Free with your Surf account

Content sourced from Wikipedia, available under CC BY-SA 4.0.

This content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.

Report