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View allAll Photos Tagged molecular
dandelionseed with a waterdrop.
nikond5300,55f2.8 nikkor macro.pb6 nikon bellows.strobe for fill in light,main light from a window.sotware for focus stacking is helicon 6.depth map mode,radius25,smoothing2.thanks everyone!:)).
This is a close-up of the underside of a plastic plant tray that I saw discarded at a garden centre.
Molecular Pharmacy received the German 「 iF」 Interior Design Award. The spiral ladder lets people think of genes, Imagination is really boundless. It is really very different, unlike traditional pharmacies. Oh ! There are also coffee drinks for sale here !
分子藥局得到德國 iF 室內設計獎。螺旋梯讓人連想到基因，想像力真的是無邊無際。它真的很不一樣，不像是傳統的藥局。 喔！這裡還有出售咖啡飲品！
Kim Dracula - Molecular Conversion
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Sᴘᴏɴsᴇʀᴇᴅ Bʏ:
☣ Outfit: Eleven - Elise @ Mainstore
☣ Pose: OMY - Marigold #1 @ Kustom9
The berries of the Virginia creeper resemble purple grapes and contain tiny crystals called oxalate crystals. These crystals are also in the leaves of Virginia creeper. If the leaves or berries are chewed they can cause irritation to the lips, mouth, tongue, and throat. (Google)
Compositionally Challenged 41
Macro in the Kitchen
Shot with a Steinheil Optronic "57 mm F 2.8" lens on a Canon EOS R5.
Here's something a little fun and different...........
This guy fired up his big block (bored out 455?), nitro burning, retro drag boat. 3000HP
The sound was absolutely ear piercing. Likely the loudest noise that I have ever heard. My eardrums felt like they ruptured, and I had pain and ringing for over an hour afterwards.
Colourful flames were throwing from the stacks.
UNFRICKIN' BELIEVABLE ! WOW !
LOVED IT !
Evening lighting with a green neon type glow.
Der Asiatische Löwe (Panthera leo persica), auch Persischer Löwe oder Indischer Löwe genannt, ist eine Unterart des Löwen. Das ursprüngliche Verbreitungsgebiet reichte bis nach Südosteuropa sowie in den Mittleren und den Nahen Osten. Er kommt heute in freier Wildbahn nur noch im indischen Staat Gujarat im Gir-Nationalpark auf der Halbinsel Kathiawar vor.
Nach molekularbiologischen Untersuchungen spaltete sich die Unterart vor 50.000 bis 100.000 Jahren vom afrikanischen Löwen ab. Insgesamt werden zurzeit zwölf Löwenunterarten unterschieden.
Der Asiatische Löwe sieht dem afrikanischen Löwen recht ähnlich, ist aber im Allgemeinen etwas kleiner. Die männlichen Tiere erreichen ein Gewicht von 160 bis maximal 190 Kilogramm, die Weibchen zwischen 110 und 120 Kilogramm. Die Schulterhöhe beträgt ca. 110 cm. Der Asiatische Löwe erreicht eine maximale Körperlänge von 290 cm. Die größte gemessene Körperlänge eines männlichen Asiatischen Löwen betrug, von der Nasen- bis zur Schwanzspitze, 292 cm.
aus Wikipedia
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The Asian Lion (Panthera leo persica), also called Persian Lion or Indian Lion, is a subspecies of the lion. The original distribution area reached as far southeastern Europe as in the Middle and the Near East. Now in the Indian state of Gujarat in the Gir National Park on the peninsula Kathiawar is the only place where asiatic lions lives in the wild.
According to molecular biological studies, the subspecies separated from the African lion 50,000 to 100,000 years ago. A total of twelve lion subspecies are currently distinguished.
The Asian lion looks quite similar to the African lion, but is generally slightly smaller. The male animals reach a weight of 160 to a maximum of 190 kilograms, the females between 110 and 120 kilograms. The shoulder height is about 110 cm. The Asian Lion reaches a maximum body length of 290 cm. The largest measured body length of a male Asian lion was 292 cm, from nose to tail.
from Wkipedia
DNA evidence and molecular studies have revealed that the round-eared elephant shrew isn't really a shrew. In fact they are more closely related to elephants than to shrews. It's funny to watch them moving too as their long back legs allow them to leap like kangaroos. A strange but cute species. :)
Pulsa L y F11 y disfruta // Click L and F11 and enjoy
Mil gracias por pasar a ver mis fotos y un millón por comentar.
Thanks for stopping to see my photos and a million for commenting.
©Reservados todos los derechos. No se permite el uso, reproducción o duplicación incluyendo electrónico sin el consentimiento por escrito.
All rights reserved. No use, reproduction or duplication including electronic is allowed without written consent.
At the base of the Judge Roybal Court House and Federal Building, stand this all aluminum
sculpture by Jonathan Borofsky !
The many holes represent the numerous molecules within man. Borofsky created several sculptures, another in the Spree River in Berlin.
Here is another image that is part of a larger project to image the entire Orion Molecular Cloud Complex at high resolution at Frosty Drew Observatory and Science Center. This image features the left star of Orion's Belt - Alnitak, the Flame Nebula, the Horsehead Nebula, and more. This project will continue over winter 2021-2022.
I captured this image over several nights in December 2020 at Frosty Drew Observatory in Charlestown, Rhode Island.
Camera: Canon Ra
Filter: L-Pro
Telescope: Astronomics AT72 ED
Astronomics 2" Field Flattener
Mount: Celestron CGEM DX
Unguided
430mm
f/6
ISO: 3200
Exposure: 120 seconds x 179 subimages
Total Integration: 14.3 hours
NGC 2359, Sharpless 2-298 or Thor's Helmet, is an emission nebula situated in the constellation of Canis Major. The central star is the Wolf-Rayet star WR7, an extremely hot star thought to be in a brief pre-supernova stage of evolution. It is similar in nature to the Bubble Nebula but interactions with a nearby large molecular cloud are thought to have contributed to the more complex shape. It lies around 11,960 distant.
Image made up from subs collected using 2 different setups. My 150mm Esprit/QHY294M and TSAPO130Q/QHY294C.
NEQ6 PRO
TSAPO130Q @F/5
QHY294C Gain 2900 -20C
STC Duo Narrowband filter
EQ6-R-PRO
150mm Esprit
QHY294M Gain 2900 -20C
Astronomik 6nm Ha and OIII narrowband filters
Acquisition time 10hrs
Processed using Pixinsight and Photoshop 6.
For Macro Monday's bread theme.
It's a crumpet, especially delicious when toasted and spread with butter and golden syrup :-)
The Pelican Nebula is an H II region associated with the North America Nebula in the constellation Cygnus. The gaseous contortions of this emission nebula bear a resemblance to a pelican, giving rise to its name. The Pelican Nebula is located nearby first magnitude star Deneb, and is divided from its more prominent neighbour, the North America Nebula, by a molecular cloud filled with dark dust. The nebula has a particularly active mix of star formation and evolving gas clouds. (Wikipedia)
Added SII and OIII subs to produce colour layer in Hubble palette to add to existing Ha luminance.
Acquisition: 31/5/15, 2/10/16
Luminance: Henley-on-Thames, UK
Colour: Chiswick, London, UK.
4 Hours total Exposure
6x1200sHa, 4x900sSII, 4x900sOIII
SII and OIII bin 2x2
Equipment:
T: Takahashi FSQ106ED
C: QSI683ws Mono CCD @-25C
F: Astronomik Ha (6nm)
M: Celestron Advanced Vx
G: QHY5-II
Software:
PHD2, Sequence Generator Pro, CCDStack, Photoshop CS6
"According to a 2020 study using a molecular clock calibrated with 27 chelicerate fossils, spiders most likely diverged from other chelicerates between 375 and 328 million years ago.
The discovery of Chimerarachne in early Late Cretaceous (Cenomanian) aged Burmese amber has also demonstrated that taxa existed until the Cretaceous that had both spinnerets, and a whip-like telson."
(Source: Wikipedia: see Evolution of spiders)
The Perseus molecular cloud, located at the junction of Taurus, Aries, and Perseus, about 1,000 light-years away from the Earth. It contains over 10,000 solar masses of gas and dust covering an area of 6 by 2 degrees, is the closest giant molecular cloud actively forming large numbers of low to intermediate-mass stars. Unlike the Orion molecular cloud, Perseus molecular cloud is almost invisible apart from two clusters, IC 348 and NGC 1333, where low-mass stars are formed.
By accumulating a very-long-time of exposure, the dust and gas show up, exhibit a complex and chaotic structure consisting of dense cloud cores surrounded by an interconnected network of filaments and sheets. Many voids surrounded by partial arcs or nearly complete rings are also seen. This complicated structure is one possible signature of supersonic turbulence.
The eastern (upper) end of the cloud is associated with IC 348 that contains several hundred young stars. Most of the star formation in IC 348 took place within the last 3 Myr, but some stars in this region formed 10 Myr ago. The apparent age spread in IC 348 may be an indication that two episodes of star formation have occurred. IC 348 appears to be an example of a region that is at or near the end of its star-forming phase.
The western (lower) portion of the Perseus cloud contains the most active region of star formation in the Perseus molecular cloud, including the NGC 1333 cluster. It contains around 150 stars with a median age of a million years, is one of the most active sites of ongoing star formation in the sky within 1500 light-years of the Sun. The molecular ridge extending south (left) from NGC 1333 contains many Herbig–Haro objects, which are bright patches of nebulosity associated with newborn stars.
Between IC 348 and NGC 1333, right in the middle of this photo, there is an area that appears pinky, which is a low-surface brightness HII region surrounded by a dust ring G159.6-18.5, which appears to lie behind the obscuration of the Perseus molecular cloud. The intense ultraviolet light emitted by the central star HD 278942 ionizes the surrounding hydrogen, giving this region its characteristic pink color. The star appears red in this photo and would have been a blue-white star if it were not obscured by dust. The presence of HD 278942 and its HII region suggests that that massive stars may have formed in the recent past within the Perseus molecular cloud.
BTW, the cloud of dust, which obscures the central star and the HII region, is called the“Flying Ghost Nebula” because of its shape.
The area to the west (lower) of the HII region looks relatively empty without too much dense dust, and particularly dark here because the extinction in this region remains high. Perhaps this dead-zone is the youngest portion of the Perseus molecular cloud, formed by the expansion of the dust ring G159.6-18.5.
There are more areas full of dense dust to the south (left) of NGC 1333, see another photo I took if you are interested: www.flickr.com/photos/steedjoy/50855451732/
Location: Galaxy Remote Observatory, Kangbao, Hebei, China
Time: October 18, 2020 - February 7, 2021
Telescope: SharpStar 150 2.8 HNT
Camera: QHY268C
Mount: iOptron CEM70/CEM60
Guide: QHYCCD OAG-M
Guide camera: QHY5L-II-M
Mosaic: 4 panels
Number of shots: 137×1000 seconds, 523×300 seconds
Cumulative exposure: 81.6 hours
Acquired by APT
Processed by PixInsight and PhotoShop
© My photographs are Copyrighted and All Rights are Reserved. They may not be used or reproduced without my explicit written permission.
Sharpless 126 (Sh2-126) and LBN 437
Credit: Giuseppe Donatiello
Sharpless 126 (Sh2-126) is a large red emission nebula in Lacerta. The source of its ionisation is the star 10 Lacertae, a blue main sequence star.
The yellow reflection nebula is designated LBN 437. It is a molecular cloud whose densest part is associated with YSOs.
This region, with its faint nebular filaments, is part of Lacerta OB1, a giant star-forming region about 1200 light-years from Earth.
Taken with 135 and 200 mm telelens array.
To use this image please first read here: www.flickr.com/people/133259498@N05/
The Corona Australis Molecular Cloud is a faint gaseous and dusty molecular cloud with many embedded reflection nebulae, including NGC 6729, NGC 6726–7 and IC 4812. A star-forming region of around 7000 Solar masses, the cloud contains Herbig–Haro objects (protostars) and some very young stars. About 430 light years away, it is one of the closest star-forming regions to the Solar System.
Takahashi FSQ106EDX4
FLI Proline 16803, CFW-5-7, Robofocus
LRGB = 380 60 50 50min = 9hrs total exposure (bin 1X1)
New Deep-Sky RGB Astronomik filters
-30C chip temp, dark frames and flats (using Aurora Flat Field Panel) applied
Focal length 530mm, FOV = 4deg X 4deg
Image scale 3.5"/pix
Guide Camera: Starlightxpress Lodestar
Comments
Data collected over three nights on 14, 18 July and 5 Aug 2018, ave seeing.
Equipment setup: www.pbase.com/strongmanmike2002/image/166437746/original