Taxonomy of Extrasolar Systems for the Main Sequence Stars

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61989592%3A15310%2F21%3A73609495" target="_blank" >RIV/61989592:15310/21:73609495 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/61389021:_____/21:00560461

Výsledek na webu

<a href="https://link.springer.com/content/pdf/10.1134/S0038094621060101.pdf" target="_blank" >https://link.springer.com/content/pdf/10.1134/S0038094621060101.pdf</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1134/S0038094621060101" target="_blank" >10.1134/S0038094621060101</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Taxonomy of Extrasolar Systems for the Main Sequence Stars

Popis výsledku v původním jazyce

In this paper we present the guidelines for an extrasolar system taxonomy. When working with an extra-solar planet database, it is very useful to have a taxonomy scale (classification). The taxonomy has to be easily interpreted and present the most relevant information about extrasolar systems. We propose the extrasolar system taxonomy scale with four parameters. The first parameter describes the actual (known) number of exoplanets in hot zone, habitable zone and cold zone of main star. We call this parameter a Zone index ZI. The second parameter is related to the Harvard classification system for the description of stellar spectral characteristics. The third parameter identifies a stellar component. The fourth parameter is a system number SN. This system number characterizes the distribution of exoplanets in extrasolar system according to their masses. According to this taxonomy scale, for example, extrasolar system 55 Cancri is 311GX12.2, Solar System is 224GX2.222.

Název v anglickém jazyce

Taxonomy of Extrasolar Systems for the Main Sequence Stars

Popis výsledku anglicky

In this paper we present the guidelines for an extrasolar system taxonomy. When working with an extra-solar planet database, it is very useful to have a taxonomy scale (classification). The taxonomy has to be easily interpreted and present the most relevant information about extrasolar systems. We propose the extrasolar system taxonomy scale with four parameters. The first parameter describes the actual (known) number of exoplanets in hot zone, habitable zone and cold zone of main star. We call this parameter a Zone index ZI. The second parameter is related to the Harvard classification system for the description of stellar spectral characteristics. The third parameter identifies a stellar component. The fourth parameter is a system number SN. This system number characterizes the distribution of exoplanets in extrasolar system according to their masses. According to this taxonomy scale, for example, extrasolar system 55 Cancri is 311GX12.2, Solar System is 224GX2.222.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10306 - Optics (including laser optics and quantum optics)

Projekt

<a href="/cs/project/EF16_026%2F0008390" target="_blank" >EF16_026/0008390: Partnerství pro excelenci v superpřesné optice</a><br>

Návaznosti

S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2021

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

SOLAR SYSTEM RESEARCH

ISSN

0038-0946

e-ISSN

—

Svazek periodika

55

Číslo periodika v rámci svazku

6

Stát vydavatele periodika

RU - Ruská federace

Počet stran výsledku

5

Strana od-do

620-624

Kód UT WoS článku

000731875700012

EID výsledku v databázi Scopus

2-s2.0-85121461628