To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

C/1911 O1 (Brooks)
C/1911 O1
Discovery
Discovered byWilliam Robert Brooks
Discovery dateJuly 21, 1911
Designations
1911 V, 1911c, Comet Brooks
Orbital characteristics
EpochOctober 11, 1911 (JD 2419320.5)
Aphelion~306.9 AU[1]
Perihelion0.489429 AU
Semi-major axis~153.7 AU
Eccentricity0.997005
Orbital period~1900 yr[1]
Inclination33.8095°
Last perihelionOctober 28, 1911
Next perihelionunknown

C/1911 O1 (Brooks), also designated 1911 V or Comet Brooks, was a bright comet discovered in July 1911 by astronomer William Robert Brooks.

It is notable for becoming a bright naked-eye object of second magnitude, with a narrow straight tail of up to thirty degrees in length and a distinct blue colour;[2] this colour seen in some comets is usually a result of the emission of carbon monoxide ions. It was also notable for uniquely being visible at the same time (mid October 1911) and in the same part of the sky as a second bright comet; this was C/1911 S3 (Beljawsky), which reached the first magnitude, had a fifteen degree tail and a bright golden-yellow appearance.[2]

C/1911 O1 (Brooks) shortly before its last perihelion, October 19, 1911.

YouTube Encyclopedic

  • 1/1
    Views:
    844
  • Oceanography

Transcription

References

  1. ^ a b Horizons output. "Barycentric Osculating Orbital Elements for Comet C/1911 O1 (Brooks)". Retrieved 2011-02-03. (Solution using the Solar System Barycenter and barycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
  2. ^ a b Bortle, J. The Bright Comet Chronicles, International Comet Quarterly, 1998

External links


This page was last edited on 22 December 2023, at 23:01
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.