Fear God (UNDER CONSTRUCTION)

FEAR GOD

Revelation 14: 7 And I saw another angel fly in the midst of heaven, having the everlasting gospel to preach unto them that dwell on the earth, and to every nation, and kindred, and tongue, and people, 7Saying with a loud voice, Fear God, and give glory to him; for the hour of his judgment is come: and worship him that made heaven, and earth, and the sea, and the fountains of waters. 8And there followed another angel, saying, Babylon is fallen, is fallen, that great city, because she made all nations drink of the wine of the wrath of her fornication. 8And there followed another angel, saying, Babylon is fallen, is fallen, that great city, because she made all nations drink of the wine of the wrath of her fornication. 9And the third angel followed them, saying with a loud voice, If any man worship the beast and his image, and receive his mark in his forehead, or in his hand, 10The same shall drink of the wine of the wrath of God, which is poured out without mixture into the cup of his indignation; and he shall be tormented with fire and brimstone in the presence of the holy angels, and in the presence of the Lamb: 11And the smoke of their torment ascendeth up for ever and ever: and they have no rest day nor night, who worship the beast and his image, and whosoever receiveth the mark of his name. 12Here is the patience of the saints: here are they that keep the commandments of God, and the faith of Jesus.

Ecclesiastes 12:13 Let us hear the conclusion of the whole matter: Fear God, and keep his commandments: for this is the whole duty of man.14For God shall bring every work into judgment, with every secret thing, whether it be good, or whether it be evil.

Universality and Cosmology

ANALYZING UNDERLYING IMPETUSES AS REFLECTED IN HISTORY (1840's-present)
Religion Civil Rights Science and Technology Space Forms of government Wars and conflicts
Crimes against humanity Literature Entertainment

Universitarianism reflected in religions, military, and politics. (1800's) III

Thursday, October 21, 2010

Extrasolar planets

Extrasolar planets

Most of the discovered extrasolar planets lie within a distance of 300 light years of the Solar System.
There are 126 known extrasolar planets for which the true mass is estimable. There are currently 100 known planets in single planetary systems and 26 known planets in 9 multiple planetary systems (3 with two planets, 3 with three, 1 with four, 1 with five[2], and 1 with six).
The majority of these transit their stars, enabling determination of the inclination of their orbits and hence the true ratio of the masses of the planets to their parent stars. Given a firm determination of the parent star's parallax and some independent means of measuring the star's mass, an absolute value can be derived for the planet's mass. Note also that eclipsing binaries can only have their masses securely determined if spectra for both objects exist, whereas a planet will not have spectra. See, for example, the introduction in ISBS. Transiting planets allows some confidence in expressing the lower limit of the spectroscopically determined mass being near to the real value, as inclination is perforce nearly edge-on to the line of sight. However, as a transiting system is still essentially a single line spectroscopic binary, it is the mass function, and not the mass, that is being determined (see section on single line spectroscopic binaries here). The mass is dependent on a solid determination of the parent star's mass, a value that is generally not well known for singleton stars.
Some extrasolar planets have been detected via astrometry, an example being Epsilon Eridani b. The planets around OGLE-2003-BLG-235L/MOA-2003-BLG-53L, OGLE-2005-BLG-071L and OGLE-2006-BLG-109L were all detected by gravitational microlensing, a method giving the ratio of the mass of the planet to that of the parent star. In these three cases, the parent star has been directly detected, enabling a determination of the actual mass of the system and confirming the companions' planetary nature. The upper limit on the detected flux from MOA-2007-BLG-400L constrains its mass to be less than 0.75 solar masses if it is a main sequence star. Planets "B" and "C" orbiting the pulsar PSR B1257+12 have their masses determined by detection of their gravitational effects on each other. 2M1207b's mass is derived from evolutionary models of substellar objects. The masses of all single stars are derived from evolutionary models.

[edit] Planet data table

Planets in multiple-planet systems are highlighted in yellow, in circumbinary orbits are green, orbiting subdwarf B stars are pink, and orbiting brown dwarfs are orange.
Star↓ Planet↓ Mass
(Compared to Jupiter)
↓
Mass Error
Margin↓
Radius
(Compared to Jupiter)
↓
Orbital
period

(days)
↓
Semimajor
axis

(AU)
↓
Orbital
eccentricity
↓
Inclination
(°)
↓
Discovery
year↓
WASP-26 b 1.02 ±0.03 1.32 2.7566 0.040 0 82.5 2010
WASP-1 b 0.89 ±0.2 1.358 2.51997 0.0382 0 83.9 2006
HAT-P-16 b 4.193 ±0.094 1.289 2.77596 0.0413 0.036 86.6 2010
Upsilon Andromedae 0.69 ±0.03 - 4.617136 0.059 0.013 ≥30 1996
Upsilon Andromedae 11.59 - - 237.7 0.822 0.224 9.3 1999
Upsilon Andromedae 10.29 - - 1302.61 2.55 0.32 23.14 1999
WASP-18 10.43 ±0.4 1.165 0.9414518 0.02047 0.0088 86 2009
HD 15082 b <4.1 - 1.497 1.2198669 0.02555 - 87.67 2010
HD 17156 b 3.212 −0.082 / +0.069 1.023 21.21688 0.1623 0.6753 86.2 2007
WASP-11/HAT-P-10 b 0.460 ±0.028 1.045 3.7224690 0.0439 0 88.5 2008
Epsilon Eridani b 1.55 ±0.24 - 2502 3.39 0.702 30.1 2000
WASP-22 b 0.56 ±0.02 1.12 3.53269 0.0468 0.023 89.2 2010
XO-3 b 11.79 ±0.59 1.217 3.1915239 0.0454 0.26 84.2 2007
HAT-P-15 b 1.946 ±0.066 1.072 10.863502 0.0964 0.190 89.1 2010
2M J044144 b 7.5 ±2.5 - - 15 - - 2010
Beta Pictoris b 8 −2 / +5 - ~6000 12 - - 2008
WASP-12 b 1.41 ±0.1 1.83 1.091435 0.0229 0.049 83.1 2008
COROT-12 b 0.917 −0.065 / +0.070 1.44 2.828042 0.04016 0.070 85.48 2010
COROT-7 b 0.0151 ±0.0025 0.150 0.853585 0.0172 0 80.1 2009
COROT-7 c 0.0264 ±0.0028 - 3.698 0.046 0 - 2009
COROT-5 b 0.467 −0.024 / +0.067 1.388 4.0378962 0.04947 0.09 85.83 2008
COROT-1 b 1.03 ±0.12 1.49 1.5089557 0.0254 0 85.1 2007
COROT-4 b 0.72 ±0.08 1.19 9.20205 0.090 0 90 2008
COROT-13 b 1.308 ±0.066 0.885 4.03519 0.051 0 88.02 2010
COROT-14 b 7.6 ±0.6 1.09 1.51214 0.027 0 79.6 2010
HAT-P-9 b 0.78 ±0.09 1.4 3.92289 0.053 0 86.5 2008
XO-4 b 1.72 ±0.2 1.34 4.12502 0.0555 0 88.7 2008
XO-5 b 1.077 ±0.037 1.089 4.1877539 0.0487 0 86.8 2008
XO-2 b 0.57 ±0.06 0.973 2.615838 0.0369 0 ≥88.58 2007
HAT-P-13 b 0.851 −0.046 / +0.029 1.28 2.91626 0.0426 0.021 83.4 2009
55 Cancri 4.8 - - 5169 5.74 0.014 53 2002
WASP-13 b 0.46 −0.0019 / +0.0017 1.21 4.35298 0.0527 0 86.9 2008
HD 80606 b 3.94 ±0.11 1.029 111.43637 0.449 0.93366 89.285 2001
WASP-19 b 1.15 ±0.08 1.31 0.7888399 0.0164 0.02 80.8 2009
OGLE-TR-211 b 1.03 ±0.2 1.36 3.67724 0.051 0 ≥87.2 2007
OGLE-TR-132 b 1.14 ±0.12 1.18 1.689868 0.0306 0 85 2003
OGLE-TR-113 b 1.32 ±0.19 1.09 1.4324757 0.0229 0 89.4 2004
OGLE-TR-111 b 0.53 ±0.11 1.067 4.0144479 0.047 0 88.1 2002
OGLE2-TR-L9 b 4.5 ±1.5 1.67 2.48553417 0.0418 - 82.47 2008
OGLE-TR-182 b 1.01 ±0.15 1.13 3.9791 0.051 0 85.7 2007
Gliese 436 b 0.072 ±0.0025 0.438 2.643904 0.02872 0.150 85.8 2004
2M1207 b 4 −1 / +6 1.5 620000 41 - - 2004
PSR B1257+12 A 0.000063 - - 25.262 0.19 0 ~50 1994
PSR B1257+12 B 0.013 - - 66.5419 0.36 0.0186 53 1992
PSR B1257+12 C 0.012 - - 98.2114 0.46 0.0252 47 1992
WASP-25 b 0.58 ±0.04 1.26 3.76483 0.0474 0 87.7 2010
HAT-P-3 b 0.599 ±0.028 0.890 2.899703 0.03894 0 87.24 2007
WASP-15 b 0.542 ±0.05 1.428 3.7520656 0.0499 0 85.5 2008
HAT-P-12 b 0.211 ±0.012 0.959 3.2130598 0.0384 0 - 2009
WASP-16 b 0.855 ±0.059 1.008 3.1186009 0.0421 0 85.22 2009
WASP-14 b 7.725 −0.67 / +0.43 1.259 2.2437704 0.037 0.0903 84.79 2008
WASP-24 b 1.032 −0.037 / +0.038 1.104 2.3412083 0.0359 0 85.71 2010
Gliese 581 e 0.006104 - - 3.14942 0.03 0 ≥30 2009
Gliese 581 b 0.0492 - - 5.36874 0.041 0 ≥30 2005
Gliese 581 c 0.01686 - - 12.9292 0.07 0.17 ≥30 2007
Gliese 581 g 0.009765 - - 36.562 0.14601 - - 2010
Gliese 581 d 0.02231 - - 66.8 0.22 0.38 ≥30 2007
Gliese 581 f 0.02205 - - 433 0.758 - - 2010
HAT-P-4 b 0.68 ±0.04 1.27 3.056536 0.0446 0 89.9 2007
Lupus-TR-3 b 0.81 ±0.18 0.89 3.91405 0.0464 0 88.3 2007
WASP-17 b 0.49 −0.056 / +0.059 1.66 3.7354417 0.051 0.129 87.8 2009
XO-1 b 0.9 ±0.07 1.3 3.941534 0.0488 0 87.7 2006
1RXS J160929.1-210524 b 8 - 1.7
~330 - - 2008
HD 147506 HAT-P-2b 9.09 ±0.24 1.157 5.6334729 0.06878 0.5171 86.72 2007
PSR B1620-26 PSR B1620-26 b 2.5 ±1 ~0.8 ~36500 23 low 55 1993
HD 149026 b 0.359 −0.021 / +0.022 0.654 2.8758887 0.04313 0 85.3 2005
GJ 1214 b 0.0179 ±0.00027 0.2415 1.5803925 0.0143 <0.27 88.62 2009
HAT-P-14 b 2.232 ±0.059 1.15 4.6267669 0.0606 0.107 83.5 2010
OGLE-2005-BLG-071L b 3.5 ±0.3 - 3600 3.6 - - 2005
OGLE-TR-10 b 0.63 ±0.14 1.26 3.10129 0.04162 0 84.5 2002
GSC 03089-00929 TrES-3 1.92 ±0.23 1.295 1.30619 0.0226 0 82.15 2007
OGLE-2006-BLG-109L b 0.727 ±0.06 - 1790 2.3 - 64 2008
OGLE-2006-BLG-109L c 0.271 ±0.022 - 4931 4.5 0.15 64 2008
GSC 02620-00648 TrES-4 0.919 ±0.073 1.799 3.553945 0.05091 0 82.86 2006
MOA-2008-BLG-310L b 0.23 ±0.05 - - 1.25 - - 2009
OGLE-2005-BLG-390L b 0.018 - - 4800 2.6 - - 2006
OGLE-2007-BLG-368L b 0.0694 - - - 3.3 - - 2009
OGLE-TR-56 b 1.29 ±0.12 1.30 1.211909 0.0225 0 78.8 2003
SWEEPS J175853.92−291120.6 SWEEPS-04 3.8 - 0.81 4.2 0.055 - ≥87 2006
SWEEPS J175902.67−291153.5 SWEEPS-11 9.7 ±5.6 1.13 1.796 0.03 - ≥84 2006
OGLE-2003-BLG-235L
/MOA-2003-BLG-53L
b 2.6 ±0.8 - - 4.3 - - 2004
OGLE-2005-BLG-169L b 0.041 - - 3100 2.7 - - 2006
MOA-2007-BLG-192L b 0.01 −0.005 / +0.015 - - 0.62 - - 2008
MOA-2007-BLG-400L b 0.9 ±0.4 - - 0.85 or 7.5 - - 2008
HAT-P-5 b 1.06 ±0.11 1.26 2.788491 0.04075 0 86.75 2007
WASP-3 b 1.76 −0.14 / +0.06 1.31 1.846834 0.0317 0 85.06 2007
COROT-11 b 2.33 ±0.34 1.43 2.99433 0.0436 0 83.17 2010
COROT-9 b 0.84 ±0.07 1.05 95.2738 0.407 0.11 >89.9 2010
COROT-6 b 2.96 ±0.34 1.166 8.887 0.0855 <0.1 - 2009
Kepler-8 b 0.603 −0.19 / +0.13 1.419 3.52254 0.0483 0 84.07 2010
Kepler-9 b 0.252 ±0.013 - 19.24 0.140 0 - 2010
Kepler-9 c 0.171 ±0.013 - 38.91 0.225 0 - 2010
Kepler-4 b 0.077 ±0.012 0.357 3.21346 0.0456 0 89.76 2010
GSC 02652-01324 TrES-1 0.61 ±0.06 1.081 3.030065 0.0393 0.135 88.2 2004
GSC 03549-02811 TrES-2 1.199 ±0.052 1.272 2.47063 0.03556 0 83.62 2006
Kepler-7 b 0.433 −0.041 / +0.040 1.478 4.885525 0.06224 0 86.5 2010
COROT-10 b 2.75 ±0.14 0.97 13.2406 0.1055 0.53 88.55 2010
COROT-8 b 0.22 ±0.03 0.57 6.21229 0.063 0 88.4 2010
COROT-2 b 3.31 ±0.16 1.465 1.7429964 0.0281 0 87.84 2007
HAT-P-7 b 1.8 −0.059 / +0.063 1.421 2.2047298 0.0379 0 84.1 2008
Kepler-6 b 0.669 −0.030 / +0.025 1.323 3.23423 0.04567 0 86.8 2010
HAT-P-11 b 0.081 ±0.009 0.422 4.8878162 0.053 0.198 88.5 2009
Kepler-5 b 2.114 ±0.064 1.431 3.54846 0.05064 0 86.3 2010
HD 189733 b 1.13 ±0.03 1.138 2.2185733 0.03099 0.00 85.76 2005
WASP-2 b 0.914 ±0.092 1.117 2.152226 0.03138 0 84.8 2006
WASP-7 b 0.96 −0.18 / +0.12 0.915 4.954658 0.0618 0 89.6 2008
HD 209458 b 0.685 −0.014 / +0.015 1.32 3.52474859 0.04707 0.07 86.677 1999
HAT-P-8 b 1.52 −0.16 / +0.18 1.5 3.07632 0.0487 0 87.5 2008
Gliese 876 d 0.021 ±0.001 - 1.93778 0.02080665 0.207 50 2005
Gliese 876 c 0.7142 ±0.0039 - 30.0881 0.12959 0.25591 48.07 2001
Gliese 876 b 2.2756 ±0.0045 - 61.1166 0.208317 0.0324 48.93 1998
Gliese 876 e 0.046 ±0.005 - 124.26 0.3343 0.055 59.5 2010
Fomalhaut b 0.054–3.0 - - ~320000 ~115 ~0.11 ~66 2008
ADS 16402 B HAT-P-1b 0.524 ±0.031 1.225 4.4652934 0.0553 0.067- 86.28 2006
HR 8799 d 10 ±3 1.2 ~36500 24 ~0 ~0 2008
HR 8799 c 10 ±3 1.2 ~69000 38 ~0 ~0 2008
HR 8799 b 7 −2 / +4 1.1 ~170000 68 ~0 ~0 2008
WASP-21 b 0.30 ±0.01 1.07 4.322482 0.052 0 88.75 2010
WASP-6 b 0.503 −0.038 / +0.019 1.224 3.361006 0.0421 0.054 88.47 2008
WASP-10 b 3.06 −0.21 / +0.23 1.08 3.0927616 0.0371 0.057 86.8 2008
WASP-4 b 1.237 −0.079 / +0.087 1.365 1.3382282 0.0230 0 89.35 2007
WASP-28 b 0.91 ±0.06 1.12 3.408821 0.0455 0.046 89.1 2010
HAT-P-6 b 1.057 ±0.119 1.33 3.852985 0.05235 0 85.51 2007
WASP-29 b 0.248 ±0.02 0.74 3.923 0.0456 0 87.96 2010
WASP-5 b 1.637 ±0.082 1.171 1.6284246 0.02729 0 85.8 2007
WASP-8 b 2.23 - 1.17 8.16 0.0793 - - 2008
Star Planet Mass
(Compared to Jupiter)
Mass Error
Margin
Radius
(Compared to Jupiter)
Orbital
period

(days)
Semimajor
axis

(AU)
Orbital
eccentricity
Inclination
(°)
Discovery
year

By Years

1833 (1) 1836 (1) 1844 (11) 1848 (3) 1850 (2) 1862 (1) 1863 (1) 1866 (1) 1867 (1) 1898 (1) 1932 (2) 1935 (1) 1938 (3) 1939 (1) 1947 (2) 1950 (1) 1958 (1) 1960 (1) 1961 (1) 1962 (1) 1964 (6) 1965 (1) 1966 (2) 1967 (2) 1968 (1) 1969 (1) 1972 (1) 1973 (1) 1976 (1) 1977 (3) 1978 (2) 1979 (15) 1980 (2) 1981 (9) 1982 (3) 1984 (1) 1986 (1) 1989 (6) 1990 (17) 1991 (10) 1992 (4) 1993 (15) 1994 (4) 1997 (2) 1999 (3) 2001 (3) 2002 (4) 2003 (2)

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