Kontent qismiga oʻtish

Fayl:Exoplanet Mass-Radius Scatter Super-Earth.png

Sahifa kontenti boshqa tillarda dastaklanmaydi.
Vikipediya, ochiq ensiklopediya

Asl fayl ‎(800 × 947 piksel, fayl hajmi: 69 KB, MIME tipi: image/png)

Ushbu fayl Vikiomborga yuklangan boʻlib, boshqa loyihalarda ham qoʻllanilishi mumkin. Uning tavsif sahifasidan olingan maʼlumot quyida keltirilgan.

Qisqa izoh

Taʼrif
English: Scatter plot of super-Earth characteristics in context showing the mass, m, and radius, r, for
 
transiting Super-Earths, (black dots),

compared with those of

 
Solar System planets (gray circles), and
 
other transiting exoplanets (gray dots)

along with

 
the distribution, n (light gray bar chart), of minimum masses (see "important note" below) of transiting and non-transiting exoplanets,

detected through 2014-04-19.

Scales indicate (log10 of) planetary mass, m, expressed as Earth masses (bottom) and Jupiter masses (top); planetary radius, r, expressed in Earth radii (left) and Jupiter radii (right); and counts n (gray ticks on right).

References lines are provided for approximate mass-radius relationships[1] for selected planetary compositions:

 
H2O - hypothetical pure water (ice) planet; any planet above this line has a significant H/He envelope;
 
75% H2O (+ 3% Fe; 22% MgSiO3) - water world;
 
67% Fe (+ 32.5% MgSiO3) - rocky terrestrial;
 
Fe - hypothetical pure iron planet, exoplanets below this line are not likely.

Exoplanet data is from the Open Exoplanet Catalogue,[2] version 4945b99. The figure shows all planets up to 10 MJ (omitting 59 more massive planets), and transiting planets up to 18 RE (omitting an additional 17 with m ≤ 10 MJ but r > 18 RE). PSR B1257+12 b (with m < 10-4 MJ), lies off to the left of the graph, and is also omitted.

Important note: This figure is intended to serve as a catalog of generally accepted candidate exoplanets using the distribution of some of their basic properties related to detection. No attempt has been made to characterize the degree of confidence (which varies widely) in the existence of a given planet or its properties. Nor is any attempt made to convey systematic errors associated with a particular method. In particular, the indicated mass, m, for an exoplanet characterized using radial velocity is the minimum mass (so that the actual distribution of masses for non-transiting planets may be shifted and "smeared" significantly to the right).

  1. ↑ Seager, S.; M. Kuchner, C. A. Hier-Majumder and B. Militzer (2007). "Mass-radius relationships for solid exoplanets". The Astrophysical Journal 669: 1279-1297. DOI:10.1086/521346. Retrieved on 2014-04-18.
  2. ↑ Open Exoplanet Catalogue (2014-04-19). Retrieved on 2014-04-19.
Sanasi
Manba Oʻzimning ishim
Muallif Aldaron, a.k.a. Aldaron
Other versions
  • Exoplanet discoveries, by year; color-coded by discovery method
    Exoplanet discoveries, by year; color-coded by discovery method
  • Scatter plot of exoplanet period and mass data; color-coded by discovery method
    Scatter plot of exoplanet period and mass data; color-coded by discovery method

Litsenziyalash

Public domain I, the copyright holder of this work, release this work into the public domain. This applies worldwide.
In some countries this may not be legally possible; if so:
I grant anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

tasvirlangan ob'ekt

tashkil etilgan

25 aprel 2014

Fayl tarixi

Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.

(eng yangi | eng eski) Koʻrib chiqish (yangiroq 10 | ) (10 | 20 | 50 | 100 | 250 | 500)
Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy12:46, 25-aprel 201412:46, 25-aprel 2014 dagi versiya uchun tasvir800 × 947 (69 KB)AldaronTidy labels.
12:53, 19-aprel 201412:53, 19-aprel 2014 dagi versiya uchun tasvir800 × 947 (68 KB)AldaronOEC catalog version 4945b99 — Update with corrections to KOI-55 b mass (using old toolchain still).
14:22, 23-yanvar 201414:22, 23-yanvar 2014 dagi versiya uchun tasvir800 × 947 (67 KB)AldaronOEC catalog version a6ef981 — Update with corrections to KOI-55 b mass (using old toolchain still).
16:08, 3-yanvar 201416:08, 3-yanvar 2014 dagi versiya uchun tasvir800 × 947 (68 KB)AldaronOEC catalog version 1f0f1dc — Refresh (using old toolchain still).
18:53, 11-oktyabr 201318:53, 11-oktyabr 2013 dagi versiya uchun tasvir800 × 947 (68 KB)AldaronUpdate with latest information from Open Exoplanets Catalog.
15:40, 15-yanvar 201315:40, 15-yanvar 2013 dagi versiya uchun tasvir800 × 947 (62 KB)AldaronUpdate after migration to OEC and addition of data through 2012.
23:33, 17-avgust 201123:33, 17-avgust 2011 dagi versiya uchun tasvir800 × 937 (45 KB)MahahahaneapneapCompressed
21:10, 21-iyul 201121:10, 21-iyul 2011 dagi versiya uchun tasvir800 × 937 (59 KB)AldaronAddition of 91 Aqr b, alf Ari b, CD-35 2722 b, CFBDS 1458 b, CHXR 73 b, CoRoT-16 b, 17 b, 18 b, 19 b, 20 b, 21 b, 23 b, DH Tau b, GJ 176 b, GJ 3634 b, Gl 785 b, GSC 06214-00210 b, HAT-P-26 b, HAT-P-27/WASP-40 b, HAT-P-28 b, HAT-P-29 b, HAT-P-30/WASP-51 b
20:07, 3-oktyabr 201020:07, 3-oktyabr 2010 dagi versiya uchun tasvir800 × 938 (46 KB)AldaronAddition of Gliese 581 f & g. Updates of MOA-2007-BLG-192-L b, WASP-29 b, HAT-P-13 b, HAT-P-14 b, HW Vir b, HW Vir c, HD 148156, Kepler-9 b, Kepler-9 c, HD 156411 b, HD 28254 b, HD 290327 b, HD 43197 b, HD 44219 b, HD 6718 b, HD 8535 b.
02:47, 29-avgust 201002:47, 29-avgust 2010 dagi versiya uchun tasvir800 × 938 (46 KB)AldaronAddition of Kepler 9 b & c, CoRoT 8 & 10 - 14 b, Gliese 876 e, HAT-P 15-25 b & 17 , HD 10180 c-h, 1RXS1609 b, 24 Sex b & c, 2M J044144 b, WASP 21, 22, 14-26, 28, 29, 31, 33, 36 & 37 b, HD, HD 102956 b, HD 109246 b, HD 145457 b, HD 200964 b & c, HD 38801 b
(eng yangi | eng eski) Koʻrib chiqish (yangiroq 10 | ) (10 | 20 | 50 | 100 | 250 | 500)

Bu faylga bogʻlangan sahifalar yoʻq.

Faylning global foydalanilishi

Ushbu fayl quyidagi vikilarda ishlatilyapti:

Metama’lumot

Bu fayl qoʻshimcha maʼlumotlarni oʻz ichiga oladi, ehtimol uni tuzish yoxud raqamlashtirish uchun raqamli kamera yoki skanerdan foydalanilgan.

Agar fayl asl holatidan oʻzgartirilgan boʻlsa, baʼzi tafsilotlar oʻzgartirilgan faylni toʻliq aks ettirmasligi mumkin.

"https://uz.wikipedia.org/wiki/Fayl:Exoplanet_Mass-Radius_Scatter_Super-Earth.png" dan olindi