Сближения астероидов с Венерой до расстояния менее 0.05 а.е. Date UT Number Name Dist Vel Size y m d h m AU km/s m 2016 01 05 21:12 2010 VQ 0.0381 4.9 8 - 17 2016 01 16 12:58 2006 LA 0.0390 33.9 462 -1033 2016 02 03 01:23 2005 SQ 0.0310 10.3 232 - 518 2016 02 08 03:20 2014 JN2 0.0412 28.3 37 - 82 2016 02 28 22:36 2009 DE1 0.0304 13.7 37 - 82 2016 03 17 07:29 2007 YP56 0.0449 19.3 18 - 41 2016 03 18 19:32 ...

... LSF_E230H_1700_da . ... STIS Model Line Spread Function vs Aperture at 170 nm Rel pixel 0.1x0.03 0.1x0.09 0.1x0.2 6x0.2 -9.915 0.0001 0.0001 0.0001 0.0001 -9.837 0.0001 0.0001 0.0001 0.0001 -9.760 0.0001 0.0001 0.0001 0.0001 -9.682 0.0001 0.0001 0.0001 0.0001 -9.605 0.0001 0.0001 0.0001 0.0002 -9.527 0.0001 0.0001 0.0002 0.0002 -9.450 0.0001 0.0002 ...

Computer Ephemeris for 2016 from DE200/LE200. Table of sidereal time. Date Sidereal time Nutation Real Mean in_alpha h m s s s s Jan 0 6 36 25.2391 25.2878 -0.0564 0.0077 1 6 40 21.7915 21.8432 -0.0545 0.0028 2 6 44 18.3435 18.3985 -0.0526 -0.0025 3 6 48 14.8961 14.9539 -0.0507 -0.0072 4 6 52 11.4497 11.5093 -0.0489 -0.0107 5 6 56 8. ... Date Sidereal time Nutation Real Mean in_alpha h m s s s s Feb 1 8 42 35. ... Date Sidereal time Nutation Real Mean in_alpha h m s s s s Mar 1 10 36 55. ...

ADD 119 04:47:14 -57:12:35 new_c #FR Clipped rms: 0.0058 Jy #FN ( 30 out of 52 channels) #MC xaxis: optical #MX Maximum: 0.145 Jy at 1251.670 km/s #MN Minimum: -0.022 Jy at 1304.887 km/s #NP Number of spectral points: 16 #CL Clipping inside range ( 0.000 , 0.000 ) Jy Moment: 0 1 2 #MM 7.577 1230.923 22.567 Robust moments: 0 1 2 #MR 5.951 1247.140 10.397 units : Jy km/s km/s km/s Width maximiser: 50% 20% #MXC Line centre : 1248.168 1235.728 #MXW ...

Thu Mar 7 10:53:21 2013 # Grid: fit_spectra.marcs (trimmed=n) # SQL: teff between 4500 and 8000 and logg between 0.0 and 5.5 and metallicity between - 3.0 and +0.5 # Mask region: 1900:10200 Filename E(B-V) RadVel teff_best logg_best m_best RMS bd02d3375sc.fits 0.0 342.0 5925.0 3.6 -2.5 0.0181 bd02d3375sc.fits 0.025 342.0 6050.0 3.8 -2.5 0.0167 bd21d0607sc.fits 0.0 -382.0 6150.0 3.9 - 1.75 0.0159 bd21d0607sc.fits 0.025 -382.0 6300.0 4.0 - ...

PSR: J2008+2513 B Scode: 2000 RAB: 20:06:28.34936 +/- 00:00:00.01100 DECB: +25:04:41.0802 +/- 00:00:00.1601 RAJ: 20:08:35.48200 +/- 00:00:00.01100 DECJ: +25:13:30.3600 +/- 00:00:00.1601 l,b: 64.055 -4.107 P: 0.589195503320000036 +/- 0.000000000060000000 Pdot: 5.395000E-15 +/- 4.000000E-18 Pepoch: 49079. DM: 60.5540 +/- 0.0090 w50: 11.00 ms 18.67 mP s400: 2.70 d,z: 3.22 -0.23 ba model d: 3.22 (model 1) L: 1.45 age: 6.24 Edot: 33.02 B: 12.26

... C) Parameter Duration a Maximum Minmum Mean DTR 1844-2004 0.0023 0 0 0 1838-2001 1886-2003 1904-2004 0.31 -0.9 0.01 0.01 Annual SE 0.0090 0 0 0 0.16 0.280 0 0 R 0.19 0.42 0.32 0.35 0.15 0.29 0.72 0.67 a 0 0 0 0 0.33 0.02 0 0 Winter SE 0 0 0 0 0.09 0.07 0 0 R 0.04 0.07 0.06 0.09 0.28 0.04 0.19 0.11 a 0 0 0 0 0.15 - 0.32 0.01 0.02 Spring SE 0 0 0 0.0010 0.08 0.14 0 0 R 0.15 0.29 0.24 0.16 ...

... Since summer 2012 it replaces the MIDAS plot engine which was used in trendPlotter before version 3.0. ... Syntax changes from MIDAS to python: . ... Compute and fit rules (identifies by COMPUTE_RULE and FIT_RULE in the config.tp_ files) have to be rewritten into Python syntax. ... Any Python statement that can be written in one line of code can be used to describe the RULES. ... One can also use multi-valued Python lists to simultaneously plot many lines on a trending plot. ... pylab.plot(ax) . ...

Общая Астрономическая Конференция > Практика > Астрономические наблюдения > Околоземные астероиды . ... Просмотр полной версии : Околоземные астероиды . ... 16.03.2009, 15:20 . ... Название ей дали 2009 DO111. ... 26 Mar 2009 0.000 13 58 58.938 + 2 44 52.36 14.3 0.0 INF 154.7 145.7 24.9 60.8 339.4 1.0119 0.0158 21.7537 4.3760 15.749" 1.529" 76.6 . 26 Mar 2009 1.000 14 0 28.182 + 2 49 20.82 14.3 0.0 INF 154.3 145.7 25.3 60.6 340.1 1.0115 0.0154 22.8118 4.5813 16.765" 1.575" 76.7 . ...

. *********** FIELD 1 ************* . *********** FIELD 2 ************* . *********** FIELD 3 ************* . *********** FIELD 4 ************* . *********** FIELD 5 ************* . *********** FIELD 6 ************* . *********** FIELD 7 ************* . *********** FIELD 8 ************* . *********** FIELD 9 ************* . *********** FIELD 10 ************* . *********** FIELD 11 ************* . *********** FIELD 12 ************* . *********** FIELD 13 ************* . *********** FIELD 14 ************* .

Instrument Science Report WFC3 2008-014 WFC3 Support in Tiny Tim Richard Hook & Felix Stoehr (ST-ECF) June 27, 2008 ABS TRACT We have extended the Tiny Tim HST point-spread function simulator so that it can now generate PSFs for the Wide Field Camera 3. ... We also introduce a web interface to Tiny Tim. ... There are two independent optical trains within WFC3, the UVIS channel with two 4096x2048 CCDs with 40mas pixels and the IR channel with a single 1024x1024 HgCdTe detector and 130mas pixels. ...

Table 1 Transition probabilities for HI k;i 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 2 2 2 2 2 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 3 4 5 6 7 ki A Aki s ;1 2 2 2 2 2 2 2 2 2 2 2 2 2 3 3 3 3 3 3 3 3 3 3 3 3 k;i 8 9 10 11 12 13 14 15 16 17 18 19 20 4 5 6 7 8 9 10 11 12 13 14 15 ki A Aki s ; 1 1215.67 1025.72 972.537 949.743 937.803 930.748 926.226 923.150 920.963 919.351 918.129 917.181 916.429 915.824 915.329 914.919 914.576 914.286 914.039 6562.80 4861.32 4340.46 4101.73 3970.07 4.699+8 5.575+7

... Летящая звезда Барнарда", как прозвали ее астрономы, обладает необычно быстрым собственным движением . ... По его расчетам, спутники З.Б. имеют массы 1.26, 0.63 и 0.89 массы Юпитера, а периоды обращения - 6.1, 12.4 и 24.8 года. ... Эти возмущения в движении З.Б. можно объяснить лишь воздействием на звезду двух спутников с массами 0.0058 и 0.0030 от массы звезды (т.е. 0.8 и 0.4 массы Юпитера). ... Публикации с ключевыми словами: Собственное движение - ближайшие звезды - звезды - Барнарда,звезда . ...

r a d i a l s t r e s s e s (top/mid/bot) MAX +1.3 @r=0.0280 +0.5 @r=0.0280 +1.1 @r=0.0498 MIN -2.4 @r=0.0597 -0.7 @r=XXXXXX -0.4 @r=0.0280 LOW_SIGMA* 99.7% 99.7% 89.1% t a n g e n t i a l s t r e s s e s (top/mid/bot) MAX +0.6 @r=0.0280 +0.4 @r=0.1172 +0.5 @r=0.1146 MIN -0.1 @r=0.0350 -4.6 @r=0.0280 -9.6 @r=0.0280 LOW_SIGMA* 88.2% 77.6% 77.4% (*) portion of surface whose stress is < .5*sigma_max axial displacements @ inner radius [micron]: mean=74.9, ptv=0.04131

. Bright Supernovae - 2009 . This data comes from IAU Circulars and occasionally more data will be provided on IAU 's Astronomical Headlines page. An archive of the 2009 updates to this page is available. This is a list of the supernovae discovered in 2009. For supernovae which are still visible, please look at the main page for the latest data. Note that Extra galactic Novae have been moved to a special Extra galactic novae page . For more information, you can look at the following Supernova Catalogs: .

Kepler-408 . KOI-1612 . KIC 10963065 . ... Масса ( солнечных масс ) . ... Радиус (солнечных радиусов) . ... планеты . ... полуось , а.е. m sin i , . масс Юпитера . радиус, . радиусов Юпитера . ... наклонение орбиты планеты i . ... Радиус эффективной земной орбиты (показана зеленым цветом) - 1.37 а.е. Расстояние до звезды оценено исходя из ее светимости и видимой звездной величины. Указан верхний предел на массу планеты Kepler-408 b ...

... 17.9 ATel #8181 4.1 (no VIZIER) 941 MASTER J080005.70+364436.4 2015 Oct 15 828 SN 17.4 ATel #8173 SA OG IIn 2.8 W,10.4 N PGC2086067,m-M=36.16 940 MASTER J203134.48+030423.4 2015 Oct 13.839 SN 16.3 ATel #8172 3.8 937 MASTER J001858.94-402211.9 2015 Oct 13.864 SN 17.0 ATel #8163 SA VS 9.7 W and 11 N PGC587150 (110Mpc) 929 MASTER J054404.79-314655.2 2015 Oct 11.046 SN 17.8 ... 02.691 PSN 18.9 ATel #4781 Kis VL SDSS r=20.3 in 4.5" 263 MASTER J131019.65+322825.0 2012 Dec. ...

g - GaAs/Alx Ga1-x As , . ... 1.2 g - GaAs/Alx Ga1-x As . ... GaAs/Alx Ga1-x As , 5 [001] D2d . ... g = g , g = g ), g ^ [001], [110], [110]. ... g - h : Ї g= 2 2 2 gz z cos2 + gxx sin2 cos2 + gyy sin2 sin2 (1.5) (1.6) h = µB B Ї 2 2 2 gz z cos2 + gxx sin2 cos2 + gyy sin2 sin2 , g - 7 1.3 g - . ... 3.5 ). 1.5 g ( ): 2 2 g 2 () = gxx cos2 + gyy sin2 (3.3) ( ) 3.3 , g [001], [110] [110] . ... Science 306,1910 (2004) [2] C. Kallin and B. I. Halperin Phys. Rev. B 30, 5655 (1984) [3] Jongso o Yo on et al., ...

start trk : onSrc master:Gr wrap:0 ast : 02:49:06.0 dut1Ms: -371 secM:10146 lmst: 17:00:22.4 mjd:54587 tolA: 10 Pos : 360.0000 19.6245 Cs:F Tm:imd Off : Rat : Rslt: 16:59:55.4- 1:15:16.8 Cs:J ha : 00:00:00.0 az deg za deg totErr cor : -0.3630 -0.0127 reqP: 359.6370 19.6118 curP: 359.6370 19.6118 errP: -0.0000 0.0000 0.0" vHel: 15.2251 vGeo:-0.0000 km/sec pend: none stat:\ OK cumO: 0.00000 0.00000 deg end start trk : onSrc master:Gr wrap:0 ast : 02:49:07.0 dut1Ms: -371 secM:10147 lmst: 17:00:23.4 mjd:54587

Астероид 1998 WT24 в декабре 2015 года. ... РДЗ Зв.в. Элонг Созв ч. м. с. њ ' а.е. а.е. m њ ----------------------------------------------------------------- Декабрь 2015 1 07h57m22.74s -05 28' 03.6 1.0185 0.0594 13.8 121.6 Mon 2 07h48m10.16s -05 14' 26.5 1.0183 0.0551 13.6 124.5 Mon 3 07h37m20.22s -04 57' 07.9 1.0179 0.0509 13.3 127.8 Mon 4 07h24m30.60s -04 35' 03.9 1.0174 0.0468 13.1 131.5 Mon 5 07h09m13.77s -04 06' 52.0 1.0167 0.0430 12.8 135.6 ...