M31n-2008-12a, 2018-11-07T19:21:38.92
RA(2000)= 00h45m28.819s DEC(2000)= +41°54’10.05”
Site location: +24:55:00N, +75:33:59E
C11 SCT/f5.5/FL 1548.6mm/D280mm, OBJCRA 00 45 28.81, OBJCDEC= +41 54 09.9, CCDT= -9.6 DegC
Binnin: 2×2, 12.9µm/12.9µm, 19’X14′, ATIK-414ex,1.66″/pix
Catalog for astrometry/photometry: UCAC4,PRISMv10
V Bessell: Exposure: 90X20=1800 secs,MAGNITUDE= 18.91 ±0.27
R Bessell: Exposure: 90X20=1800 secs, MAGNITUDE= 19.06 ±0.37
Observers: A Raj (IIA, Bengaluru, India), V.K Agnihotri (Cepheids Astronomy, RBT, INDIA)
Atel Link: http://www.astronomerstelegram.org/?read=12189
C/2018V1(Machholz-Fujikawa-Iwamoto)
Name : C/2018V1(Machholz-Fujikawa-Iwamoto)
Perihelion date : 2458456.0177 03-12-2018 12:25:29
Eccentricity : 1
Inclination (°): 143.9591
Node longitude (°): 128.729
Argument (°): 88.8273
perihelion distance (ua): 0.386714
Absolute Magnitude : 12
Activity Parameter : 4
Julian day : 2458434.44648462 -> 11-11-2018 22:42:56
RA (2000) : 12h41m23.532s DEC (2000) : -01°38’23.92”
Sun elongation (°) : 39.1
Geocentric distance (ua) : 1.036
Speed (arcsec/hour) :233.71
Angle (PA) : 84.991 °
Magnitude:10.4
RA speed : 232.9 arcsec/hour DEC : 20.4 arcsec/hour
# version=2017
# observatory
! mpcCode XXX
! name Cepheids Observatory, India
# submitter
! name V. Agnihotri
# observers
! name V. Agnihotri
# measurers
! name V. Agnihotri
# telescope
! design 0.28-m f/5.5 Schmidt-Cassegrain + CCD
! aperture 0.28
! fRatio 5.5
! detector CCD
# software
! astrometry Astrometrica 4.12.0.448
! photometry Astrometrica 4.12.0.448
permID |provID |trkSub |mode|stn |obsTime |ra |dec |rmsRA|rmsDec|astCat |mag |rmsMag|band|photCat |photAp|logSNR|seeing|exp |rmsFit|nStars|notes|remarks
|C/2018 V1 | | CCD|XXX |2018-11-12T00:01:01Z |190.442210 | -1.636303 |0.109|0.100 | UCAC4|12.85|0.086 | V| UCAC4| 7.7 |1.98 |4.1 | 60|0.11 | 15|K |
Spectrum: Comet 46P
Spectrum: 46P/2018.11.04
Cepheid Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
46P/Wirtanen
46P/Wirtanen
Date=2018/11/28, 2146 IST
Phase: 46 °
Distance: 0.1308au
Solar distance: 1.0728au
Velocity: 37.0km/s
Hourly motion: 03’08.0″ PA:23° dRA:05.24s dDec:02’53.4″
Mean J2000: RA: 02h27m19.53s DE:-22°43’00.4″
Image center R.A.=02h:28m05s.28, DEC=-22°40’18.5″
Aperture:0.2m, FL=821mm + ASI1600
Start TimeStamp : 28-11-2018|21:46IST
End TimeStamp: 28-11-2018|22:08IST
Exposure: 50sec x 26 Luminence
Pixel scale:0.955 arcsec/pixel
Orientation:Up is 82.1 degrees E of N
Modeling :
Rotational Gradient (Delta: 1.4, Alpha: 92 deg)
Larson-Sekanina (Delta: 0.0, Alpha: 45 deg)
Cepheid Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
Comet 46P/Wirtanen
Comet 46P/Wirtanen, 2018-12-23T14:25:07
0.28m+CCD, PRiSMV10
Imaged: Kuldip Vora, Measure: Vikrant Agnihotri
Cepheid Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
TCP J15360165-1642561
TCP J15360165-1642561, 2019-01-03T00:02:17.28
Astrometry: Catalog UCAC4, J2000
RA(2000)= 15h36m01.725s DEC(2000)= -16°42’58.66”
UT3.002 R MAGNITUDE= 14.27 ±0.22
UT3.004 I MAGNITUDE= 14.57 ±0.13
UT3.006 V MAGNITUDE= 14.13 ±0.10
telescope details: 0.28m Schmidt–Cassegrain+CCD
Filters Bessell BVRI
Imaged: K. Vora (Vorion Scientific Observatory, AHD, India)
Measured V. K. Agnihotri (Cepheid Observatory, RBT,India)
C/2018Y1(Iwamoto)
Name : C/2018Y1(Iwamoto), 2019-02-24T16:30:45
C8/f5.9+CCD+Lband
Perihelion date : 2458521.5258 07-Feb-19 00:37:09
Eccentricity : 0.990037
Inclination (°): 160.4015
Node longitude (°): 147.4827
Argument (°): 358.053
perihelion distance (ua): 1.286948
Absolute Magnitude : 11.5
Activity Parameter : 4
Julian day : 2458539.24919919 -> 24-Feb-19 17:58:50
RA (2000) : 06h01m05.527s DEC (2000) : +35°09’44.27”
Sun elongation (°) : 114
Geocentric distance (ua) : 0.55045
Speed (arcsec/hour) :316.4
Angle (PA) : 271.45 °
Magnitude:13.4
RA speed : -386.9 arcsec/hour DEC : 7.9 arcsec/hour
Cepheid’s Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
NGC884+869
NGC884+869
0.2m/f5.9+CCD
PRiSMv10
Cepheid Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
Comet 60P: size estimation (coma+tail)
Comet 60P: size estimation (coma+tail)
DX= 208 DY= 373 pixels
Distance (Pixels) : 427.07
Point #1 : X1=142 Y1=47
11h36m32.750s -05°54’48.85”
Point #2 : X2=349 Y2=419
11h35m45.315s -05°48’48.02”
Distance into the SKY (Angle) : 00°13’14”= 0.2167 deg
1 deg = 3.14/180 radian
0.2167 deg = 0.00378 radian
Comet geocentric distance = 0.8437 au
Estimated length of comet (coma + tail) = 0.00378 x 0.8437 = 0.00319 au
Which mean = 477217 Km
Cepheid Observatory, RBT, India
Vorion Scientific Observatory, AHD, India
Birth and Death of a Star
Birth and Death of a Star: We do not know from where to start, ice to fire or fire to ice. Keeping mind cool let us start from ice age. The cycle of birth, aging, death and rebirth of stars dominates in every galaxy, generates new elements, produces spectacular explosions called supernova and leaves “cinders, the remnants of stars behind it, which further no usually participate in cycle, called white dwarf, neutron stars, and black holes. Stars form in molecular clouds and die when they burn their fuel. Small stars end with white dwarf and large stars explode as supernova and leave neutron star and black hole behind it. In these cases, stars are supported against gravity by purely quantum effect as at the end of fuel cycle there is no outward pressure in star to hold the gravity and keep star in a particular size. First it should be known that molecular clouds are not stars because those don’t behave like black body. The clouds are so rarefied, have very low temperature and expanded up to large space. These clouds are usually made of hydrogen, carbon mono oxide and formaldehyde. The molecular clouds emit microwave radiation and keep going cool down but clouds are opaque to visible frequency range. If it so the gravity kick inward puss and the wide span cloud started shrinking, but generally we do not see it and these dust and gas cloud still hold its shape against gravity (The Eagle nebula, M16, is one its example). Now question is that, what is the extra source of energy to compensate the loss in energy by microwave radiation? The answer is cosmic energy by the near by star. Once the dense part of molecular cloud start to contract, the star birth starts gets underway. This contracting gas is called “proto star”. The minimum size of a cloud to become a proto star is called “Jeans length”. How to get that length? Very easy, equal the average kinetic energy of gas with the gravitational potential energy, so (3KT/2=GMm/R).This calculation is little wrong as the molecules on the surface leave during the process of contraction even having low velocity. The more correct calculation involved diffusion mechanism in cloud to estimate correct Jeans length. As proto star forms, slowly it gets dense and started to trap radiation and begin to behave like black body. At this point temperature rise sharply and it begins shine. Once the star forms, it will live in steady fashion for a very long time. We can not understand the death of a star until we know the mechanism of its life cycle. Here gravity works like thermostat. If at some time, suppose thermonuclear reaction gets fast, it will cause swell in the central core of star. The extra energy in terms of photon movement comes out. This reduces the temperature and density in the central core and reducing the rate of reaction. In opposite, when the central cores has less temperature and density, the gravity switch on the reaction rate by contracting the whole star and keep the fusion on.