Skip to content
Surf Wiki
Save to docs
general/astronomical-objects-discovered-in-1877

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

173 Ino

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name173 Ino
background#D6D6D6
image173 Ino VLT (2021), deconvolved.pdf
discovery_ref
discovererA. Borrelly
discovery_siteMarseille
discovered1 August 1877
mpc_name(173) Ino
alt_namesA877 PA; 1922 SB
pronounced
adjectivesInoan ( )
named_afterἸνώ *Īnṓ* (Greek mythology)
mp_categorymain-belt(middle)
Ino
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc138.75 yr (50,678 d)
aphelion3.3142 AU
perihelion2.1708 AU
semimajor2.7425 AU
eccentricity0.2085
period4.54 yr (1,659 d)
mean_anomaly307.27°
mean_motion/ day
inclination14.197°
asc_node148.18°
arg_peri228.89°
flattening0.24
mean_diameter
mass
density
rotation
albedo0.061 (calculated)
spectral_typeTholen C
SMASS Xk
B–V 0.705
U–B 0.305
abs_magnitude7.66
7.99
7.90

Ino

SMASS Xk B–V 0.705 U–B 0.305 7.99

7.90

173 Ino is a large asteroid and the parent body of the Ino family, located in the central regions of the asteroid belt, approximately 150 km in diameter. It was discovered on 1 August 1877, by French astronomer Alphonse Borrelly at Marseille Observatory in southern France, and named after the queen Ino from Greek mythology. The dark Xk-type asteroid has a rotation period of 6.15 hours.

Orbit and classification

Ino is the parent body and namesake of the Ino family (522), an asteroid family in the intermediate main belt with nearly 500 known members. The adjectival form of the asteroid name is "Inoan".

It orbits the Sun in the central main-belt at a distance of 2.2–3.3 AU once every 4 years and 6 months (1,659 days; semi-major axis of 2.74 AU). Its orbit has an eccentricity of 0.21 and an inclination of 14° with respect to the ecliptic. The body's observation arc begins at Düsseldorf-Bilk Observatory in January 1879, five months after its official discovery observation at Marseilles.

Physical characteristics

In the Tholen classification, Ino is a common carbonaceous C-type, while in the SMASS classification it is a Xk-subtype that transitions between the X-type and uncommon K-type asteroids.

Multiple photometric studies of this asteroid were performed between 1978 and 2002. The combined data gave an irregular, asymmetrical light curve with a period of 6.163 ± 0.005 hours and a brightness variation of 0.10–0.15 in magnitude. The asteroid is rotating in a retrograde direction.

Notes

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. George Stuart (1882) ''The Eclogues, Georgics, and Moretum of Virgil'', p. 271
  3. P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. ''Astronomy & Astrophysics'' 54, A56
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 173 Ino — 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