Perevod: D.Yu.Cvetkov
Poyasnenie:
Issledovatel' vnutrennego stroeniya neitronnyh zvezd
(Neutron star Interior Composition Explorer –
NICER)
nahoditsya na bortu Mezhdunarodnoi kosmicheskoi stancii. On povorachivaetsya i naklonyaetsya,
chtoby sledit' za kosmicheskimi istochnikami rentgenovskogo izlucheniya, v to vremya kak stanciya
sovershaet oborot vokrug planety Zemlya kazhdye 93 minuty.
Rentgenovskie detektory vklyuchayutsya, kogda orbita stancii prohodit po
nochnoi storone.
Yarkie dugi i petli na etoi karte vsego neba pokazyvayut, kak NICER perevodilsya ot
odnoi celi k drugoi v techenie 22 mesyacev raboty.
Dugi shodyatsya k
yarkim pyatnam
– pul'saram na rentgenovskom nebe, kotorye NICER regulyarno nablyudaet.
Pul'sary – eto vrashayushiesya neitronnye zvezdy, izluchayushie regulyarnye impul'sy rentgenovskih luchei.
Promezhutki vremeni mezhdu impul'sami nastol'ko postoyanny, chto ih mozhno ispol'zovat' dlya
navigacii
– opredeleniya skorosti i polozheniya kosmicheskogo apparata.
Eta rentgenovskaya karta vsego neba ot NICER postroena tak, chto
nebesnyi ekvator
prohodit gorizontal'no cherez centr.
1998 1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 |
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Publikacii s klyuchevymi slovami:
X-ray - rentgenovskie nablyudeniya
Publikacii so slovami: X-ray - rentgenovskie nablyudeniya | |
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