Abbreviations- M, million; k,
thousand; ly, light years; Temp, temperature; RH, relative
humidity; DP, dew point; NA, not applicable; FOV- field of view;
au- astronomical
units (1 au = distance from Sun to Earth or 93 million miles) |
Click on the images below to view a larger (1200 x 800) version in a new window. If your screen resolution is less than 1200 x 800, click on the image in the new window to view the full version. |
The Rosette Nebula,
also known as Caldwell 49, is an emission nebula
5,200 ly from Earth in the constellation
Monoceros. The nebula is about 130 ly in diameter.
The open star cluster in the middle, NGC 2244, was formed
from the nebula's matter and is less than 5 million years
old. This cluster has several O-type, super hot, stars
that generate a large amount of radiation that excites the
nebula gas. Click
on the image
to see a larger version. |
|
|
|
Object |
Rosette Nebula
(Caldwell 49) |
Distance |
5,200 ly |
Constellation |
Monoceros |
Link |
Rosette
Nebula |
|
|
Date |
January 15 - 18, 2025 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
Waning gibbous |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
2 hours; 12 x 10 min, 2 x 2 |
Green |
2 hours; 12 x 10 min, 2 x 2 |
Blue |
2 hours; 12 x 10 min, 2 x 2 |
HA |
4 hours; 24 x 10 min, 1 x 1 |
|
The Soul Nebula is an emission nebula
7,500 ly from Earth in the constellation
Cassiopeia. Along with the Heart Nebula (not seen
here), it forms a famous nebula pair referred to as the
Heart and Soul Nebula complex.
The nebula complex spans about 300
light years across and is a vast star-forming region
illuminated by the light of young, nearby stars. The stars in the region are less than a
few million years old and are only beginning their life. Click
on the image
to see a larger version. |
|
|
|
Object |
Soul Nebula
(IC 1848) |
Distance |
7,500 ly |
Constellation |
Cassiopeia |
Link |
Soul
Nebula |
|
|
Date |
January 05 - 11, 2025 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
Waxing crescent to waxing gibbous |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
3 hours; 18 x 10 min, 2 x 2 |
Green |
3 hours; 18 x 10 min, 2 x 2 |
Blue |
3 hours; 18 x 10 min, 2 x 2 |
HA |
6 hours; 36 x 10 min, 1 x 1 |
|
The California Nebula is an emission nebula 1,000 ly from Earth in the constellation
Perseus. Its name comes from its shape, which
resembles the state of California. The nebula spans about
2.5 degrees in the sky.
The red color is "glowing" hydrogen gas that is being
excited by the nearby energetic O7 star, Xi Persei, also known as Menkib, seen
at the bottom. Click
on the image
to see a larger version. |
|
|
|
Object |
California Nebula
(NGC 1499) |
Distance |
1,000 ly |
Constellation |
Perseus |
Link |
California
Nebula |
|
|
Date |
Dec 29, 2024 - Jan 02, 2025 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
Waning crescent to waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
3 hours; 18 x 10 min, 2 x 2 |
Green |
2 hours; 12 x 10 min, 2 x 2 |
Blue |
3 hours; 18 x 10 min, 2 x 2 |
HA |
4.7 hours; 28 x 10 min, 1 x 1 |
|
The Ring
Nebula (M57) is a planetary nebula 2,500 ly from Earth in the constellation
Lyra. Planetary nebula form when a star nearing the
end of its life expels a large amount of ionized gas before
becoming a white dwarf. The nebulosity seen here has
been expanding for about 1,600 years. The central star
is about 60% the mass of our Sun and 200 times brighter in
terms of its absolute magnitude. It no longer produces
its energy via nuclear fusion. Click
on the image
to see a larger version. |
|
|
|
Object |
Ring
Nebula (M57) |
Distance |
2,500 ly |
Constellation |
Lyra |
Link |
Ring Nebula |
|
|
Date |
June 01 & 02, 2024 (Tucson, AZ) |
Conditions |
Clear,
65 - 80 F |
Moon |
Waning crescent to waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
3.5 hours; 21 x 10 min, 1 x 1 |
Red |
2 hours; 12 x 10 min, 2 x 2 |
Green |
2 hours; 12 x 10 min, 2 x 2 |
Blue |
2 hours; 12 x 10 min, 2 x 2 |
HA |
NA |
|
The Rho
Ophiuchi, also known as IC 4604, is a multi-star system
360 ly from Earth in the constellation
Ophiuchus. The main stars in the system include Rho
Ophiuchi AB (binary stars seen as one large star in middle),
Rho Ophiuchi C (right) and Rho Ophiuchi DE (left, binary
stars seen as one). The star system is surrounded by a
large region of nebulosity called the Rho Ophiuchi Cloud
Complex, only a fraction of which is seen here. The
main stars in the system are hot B stars. Click
on the image
to see a larger version. |
|
|
|
Object |
Rho Ophiuchi
(IC 4604) |
Distance |
360 ly |
Constellation |
Ophiuchus |
Link |
Rho Ophiuchi Cloud Complex |
|
|
Date |
May 09 - 12, 2024 (Tucson, AZ) |
Conditions |
Clear,
60 - 80 F |
Moon |
Waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
2 hours; 12 x 10 min, 1 x 1 |
Red |
2 hours; 12 x 10 min, 2 x 2 |
Green |
2 hours; 12 x 10 min, 2 x 2 |
Blue |
2 hours; 12 x 10 min, 2 x 2 |
HA |
NA |
|
The Embryo
Nebula, also known as NGC 1333, is a reflection nebula
970 ly from Earth in the constellation
Perseus. The nebula is in the western part of the
Perseus molecular cloud and is a young region of very active
star formation. The star cluster within contains about
150 stars with a median age of about one million years.
It is associated with several dark nebula seen here. Click
on the image
to see a larger version. |
|
|
|
Object |
Embryo Nebula
(NGC 1333) |
Distance |
970 ly |
Constellation |
Perseus |
Link |
NGC 1333 |
|
|
Date |
December 12 - 15, 2023 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
Waning crescent to waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
5.5 hours; 33 x 10 min, 1 x 1 |
Red |
3.5 hours; 21 x 10 min, 2 x 2 |
Green |
3.5 hours; 21 x 10 min, 2 x 2 |
Blue |
3.5 hours; 21 x 10 min, 2 x 2 |
HA |
NA |
|
IC 405, also
known as the Flaming Star Nebula, is an emission and
reflection nebula 1500 ly from Earth in the constellation
Auriga. The nebula spans about 5 ly. This
diffuse nebula surrounds the bright hot star AE Auriga
(center) giving the impression that the star is on
fire, hence, its name. The red color is "glowing"
hydrogen gas, and the blue color is light from AE Auriga
reflected to us by dust. Click
on the image
to see a larger version. |
|
|
|
Object |
Flaming Star
Nebula (IC 405) |
Distance |
1,500 ly |
Constellation |
Auriga |
Link |
IC 405 |
|
|
Date |
December 19 - 25, 2022 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
Waning crescent to waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
1 hour; 6 x 10 min, 1 x 1 |
Red |
5 hours; 30 x 10 min, 2 x 2 |
Green |
5 hours; 30 x 10 min, 2 x 2 |
Blue |
5 hours; 30 x 10 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger image. |
M42, also
known as the Great Orion Nebula, is an emission and
reflection nebula 1300 ly from Earth in the constellation
Orion. The nebula is south of Orion's belt and spans about
24 ly. It is one of the brightest nebulas in the night
sky and is visible to the naked eye. The nebula
contains very active star formation. Click
on the image
to see a larger version. |
|
|
|
Object |
The Great Orion Nebula
(M42) |
Distance |
1,300 ly |
Constellation |
Orion |
Link |
M42 |
|
|
Date |
November 25 - 30, 2022 (Tucson, AZ) |
Conditions |
Clear,
40 - 60 F |
Moon |
New moon to first quarter |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
2 frame mosaic; 60 x 1 min per frame, 1 x 1 |
Red |
2 frame mosaic; 12 x 5 min per frame, 2 x 2 |
Green |
2 frame mosaic; 12 x 5 min per frame, 2 x 2 |
Blue |
2 frame mosaic; 12 x 5 min per frame, 2 x 2 |
HA |
NA |
Click
here
to see a larger image. |
The Horsehead Nebula is
part of the Orion Molecular Cloud Complex about 1,375 ly from Earth in
the constellation Orion. The red/pinkish glow
originates from hydrogen gas behind the dark nebula that is
ionized by ultraviolet radiation from the nearby star Sigma Orionis
(above horsehead not seen here). The dark horsehead is caused by thick dust
that blocks the light emanating from behind it. Also seen
is the Flame Nebula (red emission nebula on bottom left) and
NGC 2023 (blue reflection nebula in bottom middle). The
bright blue star is Alnitak, the left most star in Orion's
belt. Click on the link to the right to see a larger
version. |
|
Object |
Horsehead Nebula
Region |
Distance |
1,375
ly |
Constellation |
Orion |
Link |
Horsehead Nebula |
|
|
Date |
December 12 - 15, 2021 (Tucson, AZ) |
Conditions |
Clear, Temp-
38 to 52 F |
Moon |
Waning
gibbous |
Seeing |
2.0 - 4.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STX16803 |
Luminance |
2 frame mosaic; 3 x 20 min per frame, 1 x 1 |
Red |
2 frame mosaic; 3 x 20 min per frame, 2 x 2 |
Green |
2 frame mosaic; 3 x 20 min per frame, 2 x 2 |
Blue |
2 frame mosaic; 3 x 20 min per frame, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
Another image
of the Horsehead Nebula and NGC 2023 taken in 2013 with the same
telescope but a different CCD camera from the image above. |
|
Object |
Horsehead Nebula
(IC 434) |
Distance |
1,375
ly |
Constellation |
Orion |
Link |
Horsehead Nebula |
|
|
Date |
January 04 - 16, 2013 (Tucson, AZ) |
Conditions |
Clear, Temp- 23 to 46 F; DP- 3 -12 F |
Moon |
Waning to waxing crescent |
Seeing |
2.0 - 4.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
8.3 hours; 25 x 20 min, 1 x 1 |
Red |
5 hours; 15 x 20 min, 2 x 2 |
Green |
5 hours; 15 x 20 min, 2 x 2 |
Blue |
5 hours; 15 x 20 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
|
Shown is my image of the Horsehead Nebula taken with a 12.5" Ritchey-Chrétien
compared to that taken by Adam Block with a 24" Ritchey-Chrétien at
Mount Lemmon Sky Center. His image is clearly better
albeit he used a larger telescope with four times the light
gathering capacity, and imaged through darker and more
transparent skies (9,150 feet above the desert dust and light
pollution). |
M45, also
known as The Pleiades or The Seven Sisters, is an open star
cluster
440 ly from Earth in the
constellation Taurus. The nine brightest stars are
named after The Seven Sisters of Greek Mythology (Alcyone,
Electra, Maia, Merope, Taygeta, Celaeno, Sterope) along with
their two parents (Atlas, Pleione). All are hot B-type
stars. The star cluster is illuminating a dust cloud
through which it is passing creating a reflection nebulae. |
|
|
|
Object |
The Pleiades,
Seven Sisters (M45) |
Distance |
440
ly |
Constellation |
Taurus |
Link |
M45 |
|
|
Date |
November
12 - 14, 2021 (Tucson, AZ) |
Conditions |
Clear, Temp-
55 to 75 F |
Moon |
First quarter to waxing gibbous |
Seeing |
2.0 - 2.5 arc-sec |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
2 hours; 24 x 5 min, 1 x 1 |
Red |
2 hours; 24 x 5 min 2 x 2 |
Green |
2 hours; 24 x 5 min 2 x 2 |
Blue |
4 hours; 12 x 20 min 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
NGC 7000, also
known as the North American
Nebula (upper nebula), is an emission nebula 2,600 ly from Earth in the
constellation Cygnus. The shape of the nebula
resembles that of the North American continent with the Gulf
of Mexico. Also seen is the Pelican Nebula (lower
nebula, best seen in larger version, click link to right).
Both nebula are large regions of glowing hydrogen gas (HII
regions) that are being ionized by a nearby hot star emitting
ultraviolet (UV) radiation. |
|
|
|
Object |
North American Nebula
(NGC 7000) |
Distance |
2,600 ly |
Constellation |
Cygnus |
Link |
North
American Nebula |
|
|
Date |
November 03 - 06, 2021 (Tucson, AZ) |
Conditions |
Clear, Temp- 55 to 75 F |
Moon |
Waning
crescent to waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
Takahashi
TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
2 frame mosaic; 6 x 20 min per frame, 2 x 2 |
Green |
2 frame mosaic; 6 x 20 min per frame, 2 x 2 |
Blue |
2 frame mosaic; 6 x 20 min per frame, 2 x 2 |
HA |
2 frame mosaic; 6 x 20 min per frame, 1 x 1 |
Click
here
to see a larger version. |
The Veil
Nebula is a cloud of heated and ionized gas 2,400 ly from Earth in the
constellation Cygnus. It is a supernova remnant of a
star that exploded tens of thousands of years ago.
The nebula spands 3 degrees or about 6 diameters of the
moon. |
|
|
|
Object |
Veil Nebula |
Distance |
2,400 ly |
Constellation |
Cygnus |
Link |
Veil Nebula |
|
|
Date |
October
24 - 27, 2021 (Tucson, AZ) |
Conditions |
Clear, Temp-
55 to 75 F |
Moon |
Waning gibbous |
Seeing |
2.0 - 2.5 arc-sec |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
3 hours; 9 x 20 min 2 x 2 |
Green |
3 hours; 9 x 20 min 2 x 2 |
Blue |
3 hours; 9 x 20 min 2 x 2 |
HA |
4 hours; 12 x 20 min 1 x 1 |
Click
here
to see a larger version. |
NGC 281, also
known as the Pacman Nebula, is an emission nebula 9,500 ly from Earth in the
constellation Cassiopeia. The shape of the nebula
resembles that of the Pacman video game character. The
nebula is a large region of glowing hydrogen gas (HII
region) that is being ionized by a nearby hot star emitting
ultraviolet radiation. |
|
Object |
Pacman Nebula (NGC 281) |
Distance |
9,500 ly |
Constellation |
Cassiopeia |
Link |
NGC 281 |
|
|
Date |
October 30 - November 01, 2013 (Tucson) |
Conditions |
Clear, Temp-
65 to 80 F |
Moon |
Waning crescent |
Seeing |
2.0 -
3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
4.7 hours; 14 x 20 min, 1 x 1 |
Red |
3 hours; 9 x 20 min, 2 x 2 |
Green |
3 hours; 9 x 20 min, 2 x 2 |
Blue |
2 hours; 6 x 20 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
NGC 7293, also
known as the Helix
Nebula, is a planetary nebula 695 ly from Earth in the
constellation Aquarius. It is an expanding, glowing
shell of ionized gas ejected from a star late in
its life. The progenitor star (center) is now a hot
white dwarf that emits ultraviolet radiation causing
the surrounding gas to glow. |
|
Object |
Helix
Nebula (NGC 7293) |
Distance |
695 ly |
Constellation |
Aquarius |
Link |
Helix Nebula |
|
|
Date |
October 08 - 21, 2013 (Tucson, AZ) |
Conditions |
Clear, Temp-
65 to 80 F |
Moon |
Waxing crescent
to full moon |
Seeing |
2.0 -
3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
4 hours; 12 x 20 min, 1 x 1 |
Red |
2 hours; 6 x 20 min, 2 x 2 |
Green |
2 hours; 6 x 20 min, 2 x 2 |
Blue |
2 hours; 6 x 20 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
M27, also
known as the Dumbbell
Nebula, is a planetary nebula 1,250 ly from Earth in the
constellation Vulpecula. It is an expanding, glowing
shell of ionized gas ejected from a red giant star late in
its life. The progenitor star (center) is now a hot
white dwarf that emits ultraviolet radiation causing
the surrounding gas to glow. |
|
Object |
Dumbbell Nebula
(M27) |
Distance |
1,250
ly |
Constellation |
Vulpecula |
Link |
M27 |
|
|
Date |
October 01 - 04, 2013 (Tucson, AZ) |
Conditions |
Clear, Temp-
65 to 80 F |
Moon |
Waning crescent |
Seeing |
2.0 -
3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
6 hours; 18 x 20 min, 1 x 1 |
Red |
3 hours; 9 x 20 min, 2 x 2 |
Green |
3 hours; 9 x 20 min, 2 x 2 |
Blue |
3 hours; 9 x 20 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
NGC 2264, also
known as the Cone
Nebula, is a pillar of hydrogen gas and dust 2,700 ly from
Earth in the constellation Monoceros. Radiation from
hot, young stars has slowly eroded the nebula over millions
of years. Ultraviolet radiation heats the edges of the
dark cloud, releasing gas into the relatively empty region
of surrounding space. There, additional ultraviolet
radiation causes the hydrogen gas to glow, which produces
the red halo of light seen around the pillar. |
|
Object |
Cone Nebula (NGC 2264) |
Distance |
2,700
ly |
Constellation |
Monoceros |
Link |
Cone Nebula |
|
|
Date |
January 16 - February 04, 2013 (Tucson) |
Conditions |
Clear, Temp- 23 to 46 F; DP- 3 -12 F |
Moon |
Waxing to waning crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
8.3 hours; 25 x 20 min, 1 x 1 |
Red |
5 hours; 15 x 20 min, 2 x 2 |
Green |
4 hours; 12 x 20 min, 2 x 2 |
Blue |
5 hours; 15 x 20 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
Object |
Veil Nebula (NGC 6960) |
Distance |
2,600
ly |
Constellation |
Cygnus |
Link |
Veil Nebula |
|
|
Date |
September 30, 2011 (Tucson, AZ) |
Conditions |
Clear, Temp- 79 F, RH- 37%, DP- 42 F |
Moon |
Waxing crescent |
Seeing |
2.0 - 2.5 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
2 hours; 8 x 15 min, 1 x 1 |
Red |
1 hour; 4 x 15 min, 2 x 2 |
Green |
1 hour; 4 x 15 min, 2 x 2 |
Blue |
1 hour; 4 x 15 min, 2 x 2 |
HA |
NA |
|
|
|
|
Object |
Crab Nebula (M1) |
Distance |
6,300
ly |
Constellation |
Taurus |
Link |
M1 |
|
|
Date |
February 22, 2011 (Tucson, AZ) |
Conditions |
Clear, Temp- 48 F, RH- 37%, DP- 23 F |
Moon |
Waning gibbous |
Seeing |
2.0 - 2.5 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
2 hours; 12 x 10 min, 1 x 1 |
Red |
1 hour; 6 x 10 min, 2 x 2 |
Green |
1 hour; 6 x 10 min, 2 x 2 |
Blue |
1 hour; 6 x 10 min, 2 x 2 |
HA |
NA |
Click
here
to see a larger version. Click
here to see asteroid in FOV. |
|
|
|
Object |
Horsehead Nebula
Region |
Distance |
1,375
ly |
Constellation |
Orion |
Link |
Horsehead Nebula |
|
|
Date |
December 09, 2010 (Tucson, AZ) |
Conditions |
Clear, Temp- 52 F, RH- 23%, DP- 15 F |
Moon |
Waxing crescent |
Seeing |
Unknown |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
12 x 10 min; 1 x 1 |
Red |
6 x 10 min; 2 x 2 |
Green |
6 x 10 min; 2 x 2 |
Blue |
6 x 10 min; 2 x 2 |
HA |
4 x 30 min; 2 x 2 |
Click
here
to see a larger version. |
|
|
|
Object |
Cocoon
Nebula (IC 5146) |
Distance |
4,000
ly |
Constellation |
Cygnus |
Link |
Cocoon
Nebula |
|
|
Date |
September 14/15, 2010 (Tucson, AZ) |
Conditions |
Clear, Temp- 76 F, RH- 27%, DP- 39 F |
Moon |
Waxing crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
80 min 1 x 1 |
Red |
40 min 2 x 2 |
Green |
40 min 2 x 2 |
Blue |
40 min 2 x 2 |
HA |
NA |
|
|
|
|
Object |
Horsehead Nebula |
Distance |
1,600
ly |
Constellation |
Orion |
Link |
Horsehead Nebula |
|
|
Date |
February 09, 2010 (Tucson, AZ) |
Conditions |
Clear, Temp- 45 F, RH- 76%, DP- 38 F |
Moon |
Waning crescent |
Seeing |
2.0 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
60 min 1 x 1 |
Red |
30 min 2 x 2 |
Green |
30 min 2 x 2 |
Blue |
30 min 2 x 2 |
HA |
150 min 2 x 2 |
Taken by JW Freytag (his first image) |
|
|
|
Object |
Bubble Nebula
(NGC 7635) |
Distance |
7,100
ly |
Constellation |
Casseopeia |
Link |
Bubble Nebula |
|
|
Date |
October 11, 2008 (West Bloomfield, MI) |
Conditions |
Clear, Temp- 50 F, RH- 61%, DP- 37 F |
Moon |
Waxing gibbous |
Seeing |
2.5 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
NA |
Red |
60 min 2 x 2 |
Green |
60 min 2 x 2 |
Blue |
60 min 2 x 2 |
HA |
60 min 2 x 2 |
|
|
|
|
Object |
Trifid Nebula (M20) |
Distance |
5,200
ly |
Constellation |
Sagittarius |
Link |
Messier
Object 20 |
|
|
Date |
June 12, 2008 (Tucson, AZ) |
Conditions |
Clear, Temp- 83 F, RH- 15%, DP- 30 F |
Moon |
Waxing gibbous |
Seeing |
3.0 - 4.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
60 min 1 x 1 |
Red |
60 min 2 x 2 |
Green |
60 min 2 x 2 |
Blue |
60 min 2 x 2 |
HA |
NA |
Click
here
to see a larger version. |
|
|
|
Object |
Eagle Nebula (M16) |
Distance |
7,000
ly |
Constellation |
Serpens Cauda |
Link |
Messier Object 16 |
|
|
Date |
June 11, 2008 (Tucson, AZ) |
Conditions |
Clear, Temp- 87 F, RH- 22%, DP- 44 F |
Moon |
Waxing crescent |
Seeing |
2.5 - 3.0 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
60 min 1 x 1 |
Red |
NA |
Green |
60 min 2 x 2 |
Blue |
60 min 2 x 2 |
HA |
120 min 2 x 2 |
|
|
|
|
Object |
Lagoon Nebula (M8) |
Distance |
5,200
ly |
Constellation |
Sagittarius |
Link |
M8 |
|
|
Date |
September 24 & 25, 2006 (Tucson, AZ) |
Conditions |
Clear, Temp- 75 F, RH- 47%, DP- 54 F |
Moon |
Waxing crescent |
Seeing |
Unknown |
Telescope |
Takahashi TOA130 @ f7.7 |
CCD camera |
SBIG STL11000M |
Luminance |
30 min 1 x 1 |
Red |
30 min 2 x 2 |
Green |
30 min 2 x 2 |
Blue |
30 min 2 x 2 |
HA |
60 min 2 x 2 |
|
|
|
|
Object |
NGC 6914 |
Distance |
5,000
ly |
Constellation |
Cygnus |
Link |
NGC 6914 |
|
|
Date |
July 23, 2006 (West Bloomfield, MI) |
Conditions |
Clear, Temp- 64 F, RH- 65%, DP- 55 F |
Moon |
Waxing crescent |
Seeing |
2.0 - 2.5 arc-sec |
Telescope |
RCOS 12.5" Ritchey-Chretien @ f9 |
CCD camera |
SBIG STL11000M |
Luminance |
180 min 1 x 1 |
Red |
30 min 2 x 2 |
Green |
30 min 2 x 2 |
Blue |
30 min 2 x 2 |
HA |
90 min 2 x 2 |
|