Skip to content
162 Laurentia

File:162Laurentia_(Lightcurve_Inversion).png · Wikimedia Commons · See Wikimedia Commons

EntityQ141534· pop 45· linked from 12 articles

162 Laurentia

Sign in to save

Also known as (162) Laurentia, Laurentia

main-belt asteroid

In the Vinony graph

Within Vinony's link graph, 162 Laurentia is referenced by 12 other articles, and connects out to asteroid belt, Paris and day.

Vinony files it under Astronomical objects discovered in 1876, Background asteroids and Ch-type asteroids (SMASS).

Its subject is documented across 44 Wikipedia language editions.

Picture of the Day · NASA

Pathfinder on Mars

Pathfinder on Mars

2026-07-04

On July 4th, 1997, using its own array of fireworks, a parachute, and a cocoon of airbags, the Mars Pathfinder spacecraft bounced like a giant beach ball at least 15 times before it came to rest on the surface of Mars at 10:07 AM Pacific Daylight Time. After its then novel airbag-assisted landing sequence was completed, Pathfinder transmitted this color mosaic to mission operators on Earth. In the scene from another world, the Mars Sojourner robot rover is visible in the foreground, crouched on top of the unfolded Pathfinder. About the size of a large house cat, the six-wheeled, solar-powered Sojourner became the first successful Martian rover. Surrounding Pathfinder are deflated airbags and the rock-strewn terrain of the Ares Vallis floodplain. In the distance Martian hills appear against a dusty brownish sky. The Pathfinder lander was subsequently renamed the Carl Sagan Memorial Station.

via NASA APOD

Key facts

Discovered by
Paul Henry and Prosper Henry
Discovery site
Paris
Discovery date
21 April 1876
Pronunciation
/ l ɒ ˈ r ɛ n ʃ i ə /
Named after
Joseph Jean Pierre Laurent
Alternative designations
A876 HB
Minor planet category
main belt
Observation arc
113.88 yr (41596 d)
Aphelion
3.5574 AU (532.18 Gm )
Perihelion
2.4779 AU (370.69 Gm)
Semi major axis
3.0177 AU (451.44 Gm)
Orbital period sidereal
5.24 yr (1914.7 d )
Mean anomaly
300.020 °
Mean motion
0° 11 16.872 / day
Inclination
6.0977°
Longitude of ascending node
35.539°
Argument of perihelion
116.277°
Earth moid
1.49465 AU (223.596 Gm)

via Wikipedia infobox

Wikidata facts

Instance of
asteroid
Followed by
163 Erigone
Follows
161 Athor
Parent body
Sun
Minor-planet group
asteroid belt
Diameter
97.021
Orbital period
1911.481258944289
Image
162Laurentia (Lightcurve Inversion).png
Show 19 more facts
asteroid spectral type
S-type asteroid
discoverer or inventor
Prosper-Mathieu Henry
site of astronomical discovery
Paris Observatory, PSL University
time of discovery or invention
1876-04-21
albedo
0.051
Commons category
162 Laurentia
provisional designation
A876 HB
rotation period
11.8686
absolute magnitude
9.11
orbital eccentricity
0.1829986108249924
semi-major axis of an orbit
3.01426255367624
periapsis
2.462656693691693
apoapsis
3.565868413660785
orbital inclination
6.091999472938005
longitude of ascending node
35.42183602945877
argument of periapsis
115.6411808861743
mean anomaly
220.3801183082685
time of periapsis
2461741.8355200826
Sources (2)

via Wikidata · CC0

~1 min read

Encyclopedic overview

162 Laurentia is a large and dark main-belt asteroid that was discovered by the French brothers Paul Henry and Prosper Henry on 21 April 1876, and named after Joseph Jean Pierre Laurent, an amateur astronomer who discovered asteroid 51 Nemausa.

An occultation by Laurentia was observed from Clive, Alberta on 21 November 1999.

Excerpted from Wikipedia’s “162 Laurentia” article, available under the CC BY-SA 4.0 licence.

Connections

Categories