View allAll Photos Tagged messy,
Honestly I'm a messy person ^.^ I like lying around all my stuffs and actually it takes much time to clean up all of it.
Mom and Dad always complain about that bad habit. However habit can't be changed in a wink T___T
By the way, it's not my guitar(father's guitar ^^), and I don't even know how to play it >.<
Super sexy blond model with amazing curves. She wanted to do something a little sexier and naughtier than in past shoots. One of her kinky fantasies was to tease with and pour milk on herself. I like the results...do you? Was a hard shoot to concentrate and she admitted a few times during the shoot that she was getting very turned on!!
Messier 51 (colorized plates)
Credit: ESO/Dss2, Giuseppe Donatiello
RA center: 202.481° DEC center: 47.225°
Messier 51 also called The Whirlpool Galaxy (NGC 5194) is an interacting spiral galaxy in the constellation Canes Venatici. It was the first to be classified as a spiral galaxy. It is estimated to be 23 ± 4 million light-years from us.
Shae lounging around with a messy bun... much like her mom!
~
Shae is a Feeple60 Sionna with a face up by Nomyens, wig by Licht(8-9), and eyes from eyeco(10mm)
Messier 3
Credit: ESO/Dss2, Giuseppe Donatiello
FoV: 45'x45'
Colorized plate with RGB information taken with DSLR.
60 minutes integration of Messier 81. Using 10" f8 RCT and Starlight Xpress Trius 694, with an AO unit and off-axis guider.
Date: February - April 2013
Integration: 55 x 300 seconds
Canon Rebel T3i / 600D/ Kiss X5 - astro-modded.
Telescope: Officina Stellare APM 130.
Astronomik's CCD CLS Clip Filter.
Mounted on a SkyWatcher NEQ6 Pro Mount.
Guiding: Skywatcher Startravel 80/ QHY5 Guider .
www.flickr.com/photos/glasnsci/51592133704/in/dateposted/
Messier 31, the Andromeda Galaxy
date: 2nd and 3rd October, 2021
location: Ohtsuki, Yamanashi Pref., and Hara, Nagano Pref., JPN
optics: Takahshi FC-76 w/ 76D Reducer (436mm F6.3)
camera: ZWO ASI 2600MC Pro
mount: iOptron GEM45 w/ QHY5l-II and PHD2
exposure: Gain0, total 7.4hrs (1s x 64, 5sｘ214, 60s x 32, 150s x 12, 300s x 73)
Super sexy blond model with amazing curves. She wanted to do something a little sexier and naughtier than in past shoots. One of her kinky fantasies was to tease with and pour milk on herself. I like the results...do you? Was a hard shoot to concentrate and she admitted a few times during the shoot that she was getting very turned on!!
snow, ice, slush, grit, salt, water all make for very messy conditions in this part of the world
and don't even try to keep your car clean--that is a fool's errand
Messier 39 open cluster in Cygnus
About 1,010 light-years
SkyWatcher 100ED
Canon 700d
20x120s (40 mins)
Processed in PixInsight
Rotation ................. -89.447 deg
Observation start time ... 2024-05-18 23:33:04 UTC
Observation end time ..... 2024-05-19 00:31:19 UTC
Focal distance ........... 553.63 mm
Pixel size ............... 3.23 um
Field of view ............ 2d 0' 29.3" x 1d 20' 19.5"
Image center ............. RA: 21 31 33.297 Dec: +48 16 21.61 ex: +0.000342 px ey: -0.001866 px
Messier 45 - Seven Sisters
Credit: Giuseppe Donatiello
RA 3h 47m Dec +24° 07′
I obtained this image by compacting data collected during technical tests carried out last winter, exclusively with 135 and 200mm telephoto lenses.
After decades of investigations, there are still those who claim that the cirrus clouds in the Pleiades are remnants of their formation. How true will it be?
About 135 pc distant and with an estimated age of 130 ±20 Myr (Barrado y Navascués et al. 2004), M45 is certainly a young-than-average open cluster, but not as young as believed.
The higher mass members are: Alcyone, Electra, Atlas, Maia, Merope, Taygeta, Pleione and Celeno. Some of them are stars of class Be, however under 8 solar masses. It must be said, however, that some are binary and multiple systems, therefore the real masses of the individual components could be lower [A&A 425, L45-L48 (2004)]. The group mainly contains stars of class A and F, therefore between about 1 and 2.5 solar masses. Clearly there are red dwarfs and substellar objects such as numerous brown dwarfs.
Taking into account the estimated age, all stars with masses greater than 8 times the sun have already exploded as supernovae millions of years ago.
Some of the brightest stars are now in the process of evolving into red giants and some have already done so, as some massive white dwarfs have been discovered.
If we had observed the Pleiades a few million years ago, we would have seen a nice mix of white stars and red giants, as in some younger OCs.
Regardless, M45 could not have remnants of the original cloud since they usually last only a few million years before being swept away by the radiation pressure exerted by the most massive stars.
Those clouds, which many believe to be remnants of the original hydrogen cloud, are instead cirrus clouds belonging to the larger Taurus Molecular Cloud (TMC-1) that the cluster is now passing through. That cluster and cloud are not correlated can be seen from their reciprocal, almost opposing motions (Steven J. Gibson and Kenneth H. Nordsieck 2003 ApJ 589 362)
The Pleiades are moving towards the constellation of Orion and will still resist another 250 million years before completely disintegrating under the effects of the tidal forces exerted by the Milky Way.
Cirrus clouds only scatter the light of nearby stars.
A couple years since my last attempt and I am reminded how small this is and difficult to get any detail, but a somewhat better attempt than last time.
LHO, color mapped HOO
Equipment
Imaging Telescopes Or Lenses
Celestron EdgeHD 8" · Meade Starfinder 8 f/6 Newtonian OTA
Imaging Cameras
QHYCCD QHY163M · ZWO ASI1600MM
Mounts
Losmandy GM8 / GM8G · Vixen GPDX
Filters
Astronomik H-alpha CCD 12nm 2" · Baader Neodymium Moon & Skyglow 2" · SVBony OIII 7nm 2"
Accessories
Baader 2" MPCC Mark III Newton Coma Corrector (2458400A) · Celestron 0.7X Reducer EdgeHD800 (94242) · OnStep Telescope Mount Goto Controller
Software
Adobe Photoshop · Aries Productions Astro Pixel Processor (APP) · Open PHD Guiding Project PHD2 · Stefan Berg Nighttime Imaging 'N' Astronomy (N.I.N.A. / NINA)
Acquisition details
Dates:
Aug. 8, 2022 · Aug. 9, 2022
Frames:
Astronomik H-alpha CCD 12nm 2": 140×120″(4h 40′) bin 2×2
Baader Neodymium Moon & Skyglow 2": 141×120″(4h 42′) bin 2×2
Baader Neodymium Moon & Skyglow 2": 163×120″(5h 26′) -10°C bin 2×2
SVBony OIII 7nm 2": 69×120″(2h 18′) bin 2×2
Integration:
17h 6′
Darks:
100
Bias:
100
Avg. Moon age:
11.24 days
Avg. Moon phase:
86.30%
Basic astrometry details
Astrometry.net job: 6881484
RA center: 01h42m47s.8
DEC center: +51°34′40″
Pixel scale: 0.641 arcsec/pixel
Orientation: 94.769 degrees
Field radius: 0.396 degrees
Find images in the same area
Resolution: 2636x3584
File size: 8.6 MB
Data source: Backyard
Procesada con Pixinsight, telescopio de 514mm, cámara canon 5D3, Flat, bias, dark, 4 tomas de ISO 1600 x 3 min, 10 tomas de 3.5 minutos a ISO 2500
ADAD July 2014 Day 3
"Sorry it's so messy, JoLynn, but we didn't REALLY expect you to get here until next week! But these are for you and I helped!"
A globular cluster of stars in the constellation Canis Venatici
Telescope: WO ZenithStar 81 Refractor
Mount: Losmandy GM811G
Imaging Camera: ZWO ASI 2600MC Pro
Filter: Optolong L-Pro Filter
Site: Elk Grove, California, USA
Calibration Files: None
Guiding: ZWO ASI 174mm mini/Orion 60mm Guidescope/PHD2
Integration Time: 2h 6m
No of Frames: 42
Sub Exposure Time: 180 seconds
Bortle Zone: Class 6
Date Taken: April 22, 2021
Oh what a tangled web we weave. I love Oak trees at any time of year. The birds were singing and the Sun was shining today.
Highfields Stafford UK
2nd February 2014
Super sexy blond model with amazing curves. She wanted to do something a little sexier and naughtier than in past shoots. One of her kinky fantasies was to tease with and pour milk on herself. I like the results...do you? Was a hard shoot to concentrate and she admitted a few times during the shoot that she was getting very turned on!!
Image of M27, a planetary nebula in the constellation Vulpecula.
80x240"
QHY8L
GSO RC8 f/8
Sky-Watcher NEQ6-Pro
Optolong L-Enhance filter
Explanation: Close to the Great Bear (Ursa Major) and surrounded by the stars of the Hunting Dogs (Canes Venatici), this celestial wonder was discovered in 1781 by the metric French astronomer Pierre Mechain. Later, it was added to the catalog of his friend and colleague Charles Messier as M106. Modern deep telescopic views reveal it to be an island universe -- a spiral galaxy around 30 thousand light-years across located only about 21 million light-years beyond the stars of the Milky Way. Along with a bright central core, this colorful composite image highlights youthful blue star clusters and reddish stellar nurseries tracing the galaxy's spiral arms. It also shows remarkable reddish jets of glowing hydrogen gas. In addition to small companion galaxy NGC 4248 near the picture's right edge, background galaxies can be found scattered throughout the frame. M106 (aka NGC 4258) is a nearby example of the Seyfert class of active galaxies, seen across the spectrum from radio to x-rays. Active galaxies are believed to be powered by matter falling into a massive central black hole. (text from apod.nasa.gov/apod/ap090529.html)
This photo was taken march-april 2011 in village Khlepcha near Kiev, Ukraine.
Equipment: Telescope SW 25012P 1200 mm f/5, Mount WhiteSwan-180, camera QSI-583wsg, Baader MPCC. Off-axis guidecamera Orion SSAG.
RGB filter set Astronomik.
RGB: 25 frames *10 min. in each filter, bin.1x1.
Shooting conditions were not very good: Strong haze in the sky
Size 60%, crop 16:9. North at left.
Processed Pixinsight and Photoshop CS5
9 imatges de 30 segons. Capturades per Laia Sanjuan i Roger Ricart, alumnes de 2n d'ESO.
Processat a càrrec de mi mateix.
10 darks.
Telescopi LX200 GPS..
CCD Sbig ST9.
blocs.xtec.cat/oaia/2019/06/26/visita-fills-i-filles-del-...