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

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

777 Gutemberga

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
name777 Gutemberga
background#D6D6D6
discovery_ref
discovererF. Kaiser
discovery_siteHeidelberg Obs.
discovered24 January 1914
mpc_name(777) Gutemberga
alt_namesA914 BF1926 EF
A924 YB1914 TZ
named_afterJohannes Gutenberg
(German inventor)
mp_category{{plainlist
* main-belt<ref name"MPC-object" /(outer)
* background<ref name"AstDys-object" /
orbit_ref
epoch31 May 2020 (JD 2459000.5)
uncertainty0
observation_arc105.60 yr (38,570 d)
aphelion3.5831 AU
perihelion2.8745 AU
semimajor3.2288 AU
eccentricity0.1097
period5.80 yr (2,119 d)
mean_anomaly79.152°
mean_motion/ day
inclination12.942°
asc_node283.27°
arg_peri264.44°
dimensions
mean_diameter{{plainlist
* {{val65.371.03ulkm}}
* {{val65.571.9ukm}}
* {{val71.7490.095ukm}}
rotation
albedo{{plainlist
* <ref name"Mainzer-2016" /
* <ref name"SIMPS" /
* <ref name"AKARI" /
spectral_type{{plainlist
* C <ref name"Lazzaro-2004" /
* Cb <ref name"Lazzaro-2004" /
abs_magnitude9.80

A924 YB1914 TZ (German inventor)

  • main-belt(outer)
  • background
  • C (S3OS2-TH)
  • Cb (S3OS2-BB)

777 Gutemberga (prov. designation: or ) is a dark and large background asteroid, approximately 66 km in diameter, from the outer regions of the asteroid belt. It was discovered by German astronomer Franz Kaiser at the Heidelberg-Königstuhl State Observatory on 24 January 1914. The carbonaceous C-type asteroid (Cb) has a rotation period of 12.8 hours. It was named after Johannes Gutenberg (ca. 1400–1468), who introduced the printing press to Europe and started the Printing Revolution.

Orbit and classification

Gutemberga is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the outer asteroid belt at a distance of 2.9–3.6 AU once every 5 years and 10 months (2,119 days; semi-major axis of 3.23 AU). Its orbit has an eccentricity of 0.11 and an inclination of 13° with respect to the ecliptic. The body's observation arc begins at Heidelberg on 22 December 1924, almost 11 years after its official discovery observation.

Naming

This minor planet was named after Johannes Gutenberg (ca. 1400–1468), a German inventor who started the Printing Revolution with the introduction of mechanical movable type printing. Gutenberg lived and died in Mainz and the neighboring Eltville am Rhein. The was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 78). The crater Gutenberg on the Moon and the feature Rimae Gutenberg, a 223-kilometer long groove near the crater, were also named after him.

Physical characteristics

In the Tholen-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2), Gutemberga is a common, carbonaceous C-type asteroid. In the Bus–Binzel SMASS-like taxonomic variant of the S3OS2, it is a Cb-subtype, which transitions from the C-type to the somewhat brighter B-type asteroid.

Rotation period

In January 218, a rotational lightcurve of Gutemberga was obtained from photometric observations by Tom Polakis at the Command Module Observatory in Arizona. Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude ().

The result supersedes observations by Otmar Nickel of Astronomical Consortium of Mainz from February 2001, which gave a period of hours with an amplitude of magnitude (), and observations by Astronomers at the Palomar Transient Factory in California, with a period of hours and an amplitude of magnitude.().

Diameter and albedo

According to the surveys carried out by the Japanese Akari satellite, the Infrared Astronomical Satellite IRAS, and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Gutemberga measures (), () and () kilometers in diameter and its surface has an albedo of (), () and (), respectively.

The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0494 and a diameter of 65.57 kilometers based on an absolute magnitude of 9.8. Alternative mean-diameter measurements published by the WISE team include () and () with corresponding albedos of () and (). On 27 June 2008, an asteroid occultation of Gutemberga gave a best-fit ellipse dimension of (), with a poor quality rating of 1. These timed observations are taken when the asteroid passes in front of a distant star.

Notes

References

References

  1. {{GPN. 2290
  2. {{GPN. 5111
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 777 Gutemberga — 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