Usòrò:NASA-KeplerSecondLight-K2-Explained-20131211.jpg

Page contents not supported in other languages.
Shí Wikipedia, njikotá édémédé nke onyobulạ

Failụ si na nke mbu(3,899 × 3,512 pixel, ívù akwukwo orunótu: 2.71 MB, MIME nke: image/jpeg)

Failụ a si na Wikimedia Commons,enwekwara ike iji ya eme ihe na arụmarụ ọzọ. Nkọwa na ihuakwukwọ nkọwa failụ eziri na okpuru.

Mmẹkụwátá

Nkówá
English: Kepler's Second Light: How K2 Will Work

http://www.nasa.gov/kepler/keplers-second-light-how-k2-will-work/

The conception illustration depicts how solar pressure can be used to balance NASA's Kepler spacecraft, keeping the telescope stable enough to continue monitoring distant stars in search of transiting planets.

In May, Kepler lost the second of four gyroscope-like reaction wheels, ending new data collection for the original mission. A new mission concept, dubbed K2, would continue Kepler's search for other worlds, and introduce new opportunities to observe star clusters, young and old stars, active galaxies and supernovae.

Using the sun and the two remaining reaction wheels, engineers have devised an innovative technique to stabilize and control the spacecraft in all three directions of motion. This technique of using the sun as the 'third wheel' to control pointing is currently being tested on the spacecraft.

To achieve the necessary stability, the orientation of the spacecraft must be nearly parallel to its orbital path around the sun, which is slightly offset from the ecliptic, the orbital plane of Earth. The ecliptic plane defines the band of sky in which lie the constellations of the zodiac.

K2 would study a specific portion of the sky for up to 83 days, until it is necessary to rotate the spacecraft to prevent sunlight from entering the telescope. Each orbit or year would consist of approximately 4.5 unique viewing periods or campaigns.

The K2 mission concept has been presented to NASA Headquarters.

A decision to proceed to the 2014 Senior Review – a biannual assessment of operating missions – and propose for budget to fly K2 is expected by the end of 2013.

Page Last Updated: December 11th, 2013 Page Editor: Michele Johnson

NASA Official: Brian Dunbar
Ǹgụ́ụ̀bọ̀chị̀
Mkpọlọ́gwụ̀ http://www.nasa.gov/sites/default/files/k2_explained_25nov_story.jpg
Odé ákwụ́kwọ́ NASA Ames/W Stenzel

Nkwényé

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:

Nkowapụta

Tinye nkọwa otu ahịrị ihe faịlụ a na-anochi anya ya.

Ihe ndị egosiri na faịlụ a

depicts Bekee

24 Novemba 2013

Ịta nke usòrò

Bìri èhì/ogè k'ị hụ òtù ụ̀fa dị̀ m̀gbè ahụ̀.

Èhì/OgèMbọ-akaÓgólógó na asaáÒjìèmeNkwute
dị ùgbu â14:21, 12 Disemba 2013NvóÁká màkà otù ȯ dị nà 14:21, 12 Disemba 20133,899 × 3,512 (2.71 MB)DrbogdanUser created page with UploadWizard

Ihe ndị na-eso ihe eji Ihu akwụkwọ eme na faịlụ a:

Ejiji failụ zụrụ ọha

Wikis ndi a edeputara na eji kwa failụ a:

Ómárí nso