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i did it!!! i was surprised to find out that i keep only items i like and i don't like to keep items i don't like. i also walk fast and my family members like me!
the homing pigeons live here. it's all computerized now, so the guys drive their pigeons hundreds of miles away and let them out, and they fly home here, and land on that deck outside where a computer underneath registers their time of return. it's pretty cool. there are little doors where the pigeons can go back inside.
...or something like that. My new-fangled computerized Singer Quantum 9400, which I won in the Etsy/Instructables contest, next to my 1929 Singer 101. You've come a long way, baby. That said, I will never get rid of the 101. :-)
23 Dec 2025, 23:43 UT; Spotsylvania, Virginia USA. Bortle 4.5 zone.
WO Redcat51 telescope, ZWO AM5 mount and ASI2600MC camera, autoguiding, calibration frames, no filter, exp 180s, gain 100, bin 1x1, sensor -10°C, autofocus, 45 subframes. Data acquired in ASIAir. Processed in PixInsight. Image scale: 3.1 arcsec/pixel.
Clouds: scattered clouds
Transparency (AL): 5
Seeing (AL): F
Moon: illuminated xx%, age xx days
Apparent magnitude 5.7
Apparent size 1.2x0.7°
Appearance: NGC 604, the pink star forming region just left of center in the image, is worth imaging on its own with long FL setup. This wide-field image also contains many other nebulae, clusters of stars, and galaxies identified in the NGC and IC catalogs.
From Wikipedia
The Triangulum Galaxy is a spiral galaxy 2.878 million light-years (ly) from Earth in the constellation Triangulum. It is catalogued as Messier 33 or NGC 598. With the D25 isophotal diameter of 18.74 kiloparsecs (61,100 light-years), the Triangulum Galaxy is the third-largest member of the Local Group of galaxies, behind the Andromeda Galaxy and the Milky Way.
The galaxy is the second-smallest spiral galaxy in the Local Group after the Large Magellanic Cloud, which is a Magellanic-type spiral galaxy. It is believed to be a satellite of the Andromeda Galaxy or on its rebound into the latter due to their interactions, velocities, and proximity to one another in the night sky. It also has an H II nucleus.
It is sometimes informally referred to as the "Pinwheel Galaxy" by some astronomy references, in some computerized telescope software, and in some public outreach websites. However, the SIMBAD Astronomical Database, a professional database, collates formal designations for astronomical objects and indicates that Pinwheel Galaxy refers to Messier 101, which several amateur astronomy resources including public outreach websites identify by that name, and that is within the bounds of Ursa Major.
Under exceptionally good viewing conditions with no light pollution, the Triangulum Galaxy can be seen by some people with the fully dark-adapted naked eye; to those viewers, it is the farthest permanent entity visible without magnification, being about half again as distant as Messier 31, the Andromeda Galaxy. It is a diffuse, or extended, object rather than a starlike point, even without magnification, because of its physical extent.
Its observability without optical aid ranges from being relatively easily seen by people using direct vision in deep rural locations under a dark, clear, transparent sky, to requiring use of averted vision by observers in locations beyond the suburbs in shallow rural areas under good viewing conditions. It is one of the reference objects of the Bortle Dark-Sky Scale.
Crumey has shown that although the total apparent V-magnitude of M33 is 5.72, it has an effective visual magnitude of approximately 6.6, meaning that a precondition for visibility is that the observer can see stars at least as faint as that latter figure. This is fainter than many people are able to see, even at a very dark site.
The Triangulum Galaxy was probably discovered by the Italian astronomer Giovanni Battista Hodierna before 1654. In his work De systemate orbis cometici; deque admirandis coeli caracteribus ("About the systematics of the cometary orbit, and about the admirable objects of the sky"), he listed it as a cloud-like nebulosity or obscuration and gave the cryptic description, "near the Triangle hinc inde". This is in reference to the constellation Triangulum as a pair of triangles. The magnitude of the object matches M33, so it is most likely a reference to the Triangulum Galaxy.
The galaxy was independently discovered by Charles Messier on the night of August 25–26, 1764. It was published in his Catalog of Nebulae and Star Clusters (1771) as object number 33; hence the name M33. When William Herschel compiled his extensive catalog of nebulae, he was careful not to include most of the objects identified by Messier. However, M33 was an exception, and he cataloged this object on September 11, 1784, as H V-17.
Herschel also cataloged the Triangulum Galaxy's brightest and largest H II region (diffuse emission nebula containing ionized hydrogen) as H III.150 separately from the galaxy itself; the nebula eventually obtained NGC number 604. As seen from Earth, NGC 604 is located northeast of the galaxy's central core. It is one of the largest H II regions known, with a diameter of nearly 1500 light-years and a spectrum similar to that of the Orion Nebula. Herschel also noted three other smaller H II regions (NGC 588, 592, and 595).
It was among the first "spiral nebulae" identified as such by Lord Rosse in 1850. In 1922–23, John Charles Duncan and Max Wolf discovered variable stars in the nebulae. Edwin Hubble showed in 1926 that 35 of these stars were classical Cepheids, thereby allowing him to estimate their distances. The results were consistent with the concept of spiral nebulae being independent galactic systems of gas and dust, rather than just nebulae in the Milky Way.
The Triangulum Galaxy is the third largest member of the Local Group of galaxies. It has a diameter measured through the D25 standard - the isophote where the surface brightness of the galaxy reaches 25 mag/arcsec2, to be about 18.74 kiloparsecs (61,100 light-years),[5] making it roughly 70% the size of the Milky Way. It may be a gravitationally bound companion of the Andromeda Galaxy. Triangulum may be home to 40 billion stars, compared to 400 billion for the Milky Way and 1 trillion for Andromeda.
The disk of Triangulum has an estimated mass of (3–6) billion solar masses, while the gas component is about 3.2 billion solar masses. Thus, the combined mass of all baryonic matter in the galaxy may be 10 billion solar masses. The contribution of the dark matter component out to a radius of 55×103 ly (17 kpc) is equivalent to about 50 billion solar masses.
Estimates of the distance from the Milky Way to the Triangulum Galaxy vary depending on the measurement technique. The average of 102 distance estimates published since 1987 gives a distance modulus of 24.69, or .883 Mpc (2.878 Mly). In general, measurements range from 2.380×106 to 3.070×106 ly (730 to 941 kpc) (or 2.38 to 3.07 Mly), with most estimates since the year 2000 lying in the middle portion of this range. This makes the Triangularum Galaxy slightly more distant than the Andromeda Galaxy (at 2.54 Mly). The Triangulum Galaxy is around 0.75 Mly from the Andromeda Galaxy.
Using the Cepheid variable method, an estimate of 2.770×106 ± 0.130×106 ly (849 ± 40 kpc) was achieved in 2004. In the same year, the tip of the red-giant branch (TRGB) method was used to derive a distance estimate of 2.590×106 ± 0.080×106 ly (794 ± 25 kpc). In 2006, a group of astronomers announced the discovery of an eclipsing binary star in the Triangulum Galaxy. By studying the eclipses of the stars, astronomers were able to measure their sizes. Knowing the sizes and temperatures of the stars, they were able to measure the absolute magnitude of the stars. When the visual and absolute magnitudes are known, the distance to the star can be measured. The stars lie at the distance of 3.070×106 ± 0.240×106 ly (941 ± 74 kpc). Measurements of blue supergiants in 2009 indicated a distance of 940 kpc (3.2 Mly) In 2023, the distance to M33 was measured to be 840 ± 11 kpc using Cephid photometry.
The Triangulum Galaxy is a source of H2O maser emission. In 2005, using observations of two water masers on opposite sides of Triangulum via the VLBA, researchers were for the first time able to estimate the angular rotation and proper motion of Triangulum. A velocity of 190 ± 60 km/s relative to the Milky Way was computed, which means Triangulum is moving towards Andromeda Galaxy and suggesting it may be a satellite of the larger galaxy (depending on their relative distances and margins of error).
In 2004, evidence was announced of a clumpy stream of hydrogen gas linking the Andromeda Galaxy with Triangulum, suggesting that the two may have tidally interacted in the past. This discovery was confirmed in 2011. A distance of less than 300 kiloparsecs between the two supports this hypothesis.
The Pisces Dwarf (LGS 3), one of the small Local Group member galaxies, is located 2,022×103 ly (620 kpc) from the Sun. It is 20° from the Andromeda Galaxy and 11° from Triangulum. As LGS 3 lies at a distance of 913×103 ly (280 kpc) from both galaxies, it could be a satellite galaxy of either Andromeda or Triangulum. LGS 3 has a core radius of 483 ly (148 pc) and 26 million solar masses.
Pisces VII/Triangulum (Tri) III may be another satellite of Triangulum.
...the Triangulum Galaxy is classified as type SA(s)cd. The S prefix indicates that it is a disk-shaped galaxy with prominent arms of gas and dust that spiral out from the nucleus—what is commonly known as a spiral galaxy. The A is assigned when the galactic nucleus lacks a bar-shaped structure, in contrast to SB class barred spiral galaxies. American astronomer Allan Sandage's "(s)" notation is used when the spiral arms emerge directly from the nucleus or central bar, rather than from an inner ring as with an (r)-type galaxy. Finally, the cd suffix represents a stage along the spiral sequence that describes the openness of the arms. A rating of cd indicates relatively loosely wound arms.
This galaxy has an inclination of 54° to the line of sight from Earth, allowing the structure to be examined without significant obstruction by gas and dust. The disk of the Triangulum Galaxy appears warped out to a radius of about 8 kpc. There may be a halo surrounding the galaxy, but there is no bulge at the nucleus. This is an isolated galaxy and there are no indications of recent mergers or interactions with other galaxies, and it lacks the dwarf spheroidals or tidal tails associated with the Milky Way.
Triangulum is classified as unbarred, but an analysis of the galaxy's shape shows what may be a weak bar-like structure about the galactic nucleus. The radial extent of this structure is about 0.8 kpc.
The nucleus of this galaxy is an H II region, and it contains an ultraluminous X-ray source with an emission of 1.2 × 1039 erg s−1, which is the most luminous source of X-rays in the Local Group of galaxies. This source is modulated by 20% over a 106-day cycle. However, the nucleus does not appear to contain a supermassive black hole, as a best-fit value of zero mass and an upper limit of 1,500 M☉ is placed on the mass of a central black hole based on models and the Hubble Space Telescope (HST) data. This is significantly lower than the mass expected from the velocity dispersion of the nucleus and far below any mass predicted from the disk kinematics. This may suggest that supermassive black holes are associated only with galaxy bulges instead of with their disks. Assuming that the upper limit of the central black hole is correct, it would be rather an intermediate-mass black hole.
The inner part of the galaxy has two luminous spiral arms, along with multiple spurs that connect the inner to the outer spiral features. The main arms are designated IN (north) and IS (south).
In the central 4′ region of this galaxy, atomic gas is being efficiently converted to molecular gas, resulting in a strong spectral emission of CO. This effect occurs as giant molecular clouds condense out of the surrounding interstellar medium. A similar process is taking place outside the central 4′, but at a less efficient pace. About 10% of the gas content in this galaxy is in the molecular form.
Star formation is taking place at a rate that is strongly correlated with local gas density, and the rate per unit area is higher than in the neighboring Andromeda Galaxy. (The rate of star formation is about 3.4 solar masses Gyr−1 pc−2 in the Triangulum Galaxy, compared to 0.74 in Andromeda.) The total integrated rate of star formation in the Triangulum Galaxy is about 0.45 ± 0.1 solar masses per year. It is uncertain whether this net rate is currently decreasing or remaining constant.
Based on analysis of the chemical composition of this galaxy, it appears to be divided into two distinct components with differing histories. The inner disk within a radius of 30×103 ly (9 kpc) has a typical composition gradient that decreases linearly from the core. Beyond this radius, out to about 82×103 ly (25 kpc), the gradient is much flatter. This suggests a different star formation history between the inner disk and the outer disk and halo, and may be explained by a scenario of "inside-out" galaxy formation. This occurs when gas is accumulated at large radii later in a galaxy's life space, while the gas at the core becomes exhausted. The result is a decrease in the average age of stars with increasing radius from the galaxy core.
Using infrared observations from the Spitzer Space Telescope, a total of 515 discrete candidate sources of 24 μm emission within the Triangulum Galaxy have been catalogued as of 2007. The brightest sources lie within the central region of the galaxy and along the spiral arms.
Many of the emission sources are associated with H II regions of star formation. The four brightest HII regions are designated NGC 588, NGC 592, NGC 595, and NGC 604. These regions are associated with molecular clouds containing 120,000 to 400,000 solar masses. The brightest of these regions, NGC 604, may have undergone a discrete outburst of star formation about three million years ago. This nebula is the second most luminous HII region within the Local Group of galaxies, at 45 ± 15 million times the luminosity of the Sun.[49] Other prominent HII regions in Triangulum include IC 132, IC 133, and IK 53.
The northern main spiral arm contains four large HII regions, while the southern arm has greater concentrations of young, hot stars. The estimated rate of supernova explosions in the Triangulum Galaxy is 0.06 Type Ia and 0.62 Type Ib/Type II per century. This is equivalent to a supernova explosion every 147 years, on average. As of 2008, a total of 100 supernova remnants have been identified in the Triangulum Galaxy, the majority of which lie in the southern half of the spiral galaxy. Similar asymmetries exist for H I and H II regions, plus highly luminous concentrations of massive, O type stars. The center of the distribution of these features is offset about two arc minutes to the southwest. M33 being a local galaxy, the Central Bureau for Astronomical Telegrams (CBAT) tracks novae in it along with M31 and M81.
About 54 globular clusters have been identified in this galaxy, but the actual number may be 122 or more. The confirmed clusters may be several billion years younger than globular clusters in the Milky Way, and cluster formation appears to have increased during the past 100 million years. This increase is correlated with an inflow of gas into the center of the galaxy. The ultraviolet emission of massive stars in this galaxy matches the level of similar stars in the Large Magellanic Cloud.
In 2007, a black hole about 15.7 times the mass of the Sun was detected in this galaxy using data from the Chandra X-ray Observatory. The black hole, named M33 X-7, orbits a companion star which it eclipses every 3.5 days. It is the largest stellar mass black hole known.
Unlike the Milky Way and Andromeda galaxies, the Triangulum Galaxy does not appear to have a supermassive black hole at its center. This may be because the mass of a galaxy's central supermassive black hole correlates with the size of the galaxy's central bulge, and unlike the Milky Way and Andromeda, the Triangulum Galaxy is a pure disk galaxy with no bulge.
As mentioned above, M33 is linked to M31 by several streams of neutral hydrogen and stars, which suggests that a past interaction between these two galaxies took place from 2 to 8 billion years ago, and a more violent encounter will occur 2.5 billion years in the future.
The fate of M33 was uncertain in 2009 beyond seeming to be linked to its larger neighbor M31. Suggested scenarios include being torn apart and absorbed by the greater companion, fueling the latter with hydrogen to form new stars; eventually exhausting all of its gas, and thus the ability to form new stars; or participating in the collision between the Milky Way and M31, likely ending up orbiting the merger product and fusing with it much later. Two other possibilities are a collision with the Milky Way before the Andromeda Galaxy arrives or an ejection out of the Local Group. Astrometric data from Gaia appears in 2019 to rule out the possibility that M33 and M31 are in orbit. If correct, M33 is on its first infall proper into the Andromeda Galaxy (M31).
This was actually a small trip to HEB. I bought a ton of these warm whites and multicolored from HEB in 2010. They got down to $2/box. Each strand has 50 LED lights.
Taken at the 1st Annual OLC (On Line Computerized) Cross Country Soaring Camp at Moriarty, New Mexico.
Some Assembly Required.
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It makes a computerized life for them. AGXL gives immense pool of assets to #learning. It is a main #Educational #website for #students.
Staff members at Medical Maintenance Operations Division-Tracy inspect a computerized tomography system that recently arrived to the depot for recapitalization. (Photo by Ellen Crown, US Army.)
Read the full story online now at: mrmc.amedd.army.mil/index.cfm?pageid=media_resources.arti...
Story written by: Ellen Crown, USAMMA Public Affairs
Taken At The First Annual OLC (On Line Computerization) Cross Country Soaring Camp At Moriarty, New Mexico,
These Are The USAF Academy Glider Team Trailers and The Art Work On Them. Five USAF Academy Gliders Participated in The Cross Country Soaring Camp.
Ship's engineer is kept busy with the new computerized, environmentally-friendly Caterpillar diesel prime movers. The telegraph is probably mostly ornamental now.
In the computerized age, online stages have changed the manner in which we approach wellness, offering a plenty of methods and devices to support inspiration and upgrade our gym experience. Among these, objective setting and progress following stand apart as crucial systems for driving achievement. How about we dive into how these procedures can be utilized to supercharge your inspiration in the online wellness domain:
Objective Setting:
Setting clear, noteworthy objectives is the groundwork of any fruitful wellness venture. When done actually, objective setting gives guidance, reason, and inspiration to your exercises. This is the way to outfit the force of objective setting in the online wellness space:
•Particularity: Characterize your objectives with lucidity and explicitness. Rather than unclear goals like "getting in shape," go for the gold, for example, shedding 10 pounds, running a 5k race, or deadlifting your body weight. Explicit objectives give you a reasonable objective to hold back nothing, simpler to follow progress and remain propelled.
•Quantifiability: Make your objectives quantifiable so you can keep tabs on your development after some time. Whether it's following your weight, body estimations, exercise execution, or perseverance levels, having quantifiable measurements permits you to see unmistakable outcomes and celebrate achievements en route.
•Feasibility: Put forth objectives that are testing yet achievable in view of your ongoing wellness level, assets, and time period. Try not to set ridiculous assumptions that could set you up for frustration or burnout. All things considered, break down bigger objectives into more modest, reasonable advances that you can accomplish steadily.
•Significance: Guarantee that your objectives are actually significant and pertinent to your qualities, interests, and needs. Adjust your wellness objectives to your more extensive goals and way of life, so you feel truly put resources into seeking after them.
•Time-bound: Lay out a course of events or cutoff time for accomplishing your objectives to make a need to keep moving and responsibility. Setting cutoff times forestalls delaying and spurs you to make a predictable move towards your objectives.
Progress Following:
Whenever you've defined your objectives, keeping tabs on your development is fundamental for remaining responsible and propelled. Online stages offer different devices and techniques to really keep tabs on your development:
•Wellness Applications: Use wellness following applications and stages to log your exercises, screen your nourishment, and keep tabs on your development over the long run. Numerous applications offer highlights like exercise plans, practice exhibitions, progress graphs, and objective setting instruments to assist you with remaining coordinated and propelled.
•Wearable Gadgets: Put resources into wearable wellness trackers, for example, smartwatches or action screens, to screen your everyday action levels, pulse, and calorie consumption. Wearable gadgets give continuous input on your wellness endeavors and can act as strong inspirations to remain dynamic and responsible.
•Online Diaries and Calculation sheets: Keep a computerized diary or calculation sheet to record your exercises, sustenance, and other important information. Following your everyday exercises, accomplishments, and misfortunes permits you to distinguish designs, evaluate your headway, and settle on informed conclusions about your wellness process.
•Visual Advancement Photographs: Take progress photographs at customary stretches to follow changes in your body after some time outwardly. Contrasting when photographs can be a strong inspiration, helping you to remember how far you've come and rousing you to continue to push towards your objectives.
•Online Coaching Stages: Assuming that you're working with an online mentor, exploit the advancement following highlights incorporated into their coaching stage. Numerous online coaching in lisburn offer apparatuses for following exercises, logging nourishment, speaking with your mentor, and getting criticism on your advancement.
Using Inspirational Instruments and Assets
In the powerful universe of online wellness, an abundance of persuasive devices and assets are promptly accessible to light your enthusiasm and keep you driven towards your objectives. We should investigate probably the best ways of tackling these assets:
1. Moving Substance: Search out inspirational substance that impacts you, whether it's motivating statements, examples of overcoming adversity, or instructive articles. Follow wellness powerhouses, mentors, and competitors via web-based entertainment stages like Instagram, YouTube, and TikTok for a constant flow of support and motivation.
2. Perception Procedures: Use representation methods to intellectually practice your exercises and envision yourself accomplishing your wellness objectives. Shut your eyes and distinctively envision yourself pulverizing your exercises, getting through levels, and arriving at new achievements. Perception can support your certainty and inspiration, making it more straightforward to remain on track and focused on your wellness process.
3. Positive Certifications: Integrate positive insistences into your day to day daily practice to develop a positive outlook and lift your self-assurance. Rehash confirmations, for example, "I'm solid," "I'm skilled," and "I'm gaining ground consistently" to support positive convictions about yourself and your capacity to accomplish your wellness objectives.
4. Objective Setting and Progress Following: Set explicit, quantifiable, and attainable objectives for yourself, and keep tabs on your development routinely to remain propelled and responsible. Separate your bigger objectives into more modest, significant stages, and commend your accomplishments en route. Utilize online instruments and applications to follow your exercises, sustenance, and progress towards your objectives.
5. Responsibility Accomplices: Find a responsibility accomplice or exercise mate who shares your wellness objectives and can assist with keeping you persuaded and on target. Whether it's a companion, relative, or individual gym-participant, having somebody to impart your advancement to and consider you responsible can offer important help and support.
Integrating Assortment and Fun into Exercises
To keep your exercises crisp, invigorating, and charming, integrating assortment and fun into your routine is fundamental. Here are an imaginative ways of brightening up your exercises and keep fatigue under control:
1. Attempt New Exercises: Investigate various kinds of exercises and exercises to keep your routine intriguing and testing. Whether it's yoga, Pilates, kickboxing, or dance classes, attempting new exercises can invigorate your body and psyche, forestall weariness, and assist you with finding better approaches to remain dynamic.
2. Stir Up Your Daily practice: Fluctuate your exercises by integrating various activities, hardware, and preparing modalities. Explore different avenues regarding bodyweight works out, free loads, obstruction groups, and gym machines to target different muscle gatherings and keep your exercises assorted and locking in.
3. Set Fun Difficulties: Challenge yourself with fun wellness challenges that stretch your boundaries and test your perseverance. Whether it's a board challenge, a squat test, or a virtual race, defining objectives and contending with yourself or others can add energy and inspiration to your exercises.
4. Get Outside: Take your exercises outside and partake in the advantages of outside air, daylight, and normal landscape. Go for a run or climb in the recreation area, do bodyweight practices at the ocean side, or attempt open air exercises like cycling, kayaking, or rock moving to mix it up and experience to your exercises.
5. Bunch Exercises: Join bunch wellness classes or exercise with companions to add a social component to your exercises and keep you inspired. Bunch exercises give fellowship, responsibility, and inspiration, making it simpler to remain predictable and focused on your wellness objectives.
In outline, using persuasive devices and assets, alongside integrating assortment and fun into your exercises, are fundamental techniques for remaining roused and focused on your wellness process. Whether you're looking for motivation, responsibility, or better approaches to challenge yourself, there are innumerable assets and exercises accessible to assist you with remaining drew in, persuaded, and amped up for your wellness objectives. Try different things with various methods, find what turns out best for you, and partake in the excursion towards a better, more joyful you.
New milking parlour. Double 8 stalls. Computerized, even knows how much the cow ate the night before! / Nouvelle salle de traite.
Something to remember is usually that will soon enough your hard work needs to be computerized and you should employ a program completed to the extent that you just will not need to concern yourself with points. The ultimate way to begin accomplishing this is to get aid from the virtual assistant that could check out emails, style mails and get the calls when you are very occupied. You'll be able to use this kind of asst on the web or perhaps possibly discover one inside where you live. A lot of people produce the mistake together with considering they are able to go into this kind of area instead of need virtually any aid, that's whenever they commonly don't succeed.
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All In A Day - This computerized sign was scheduled for freeway installation (construction barrel heaven) in the near future. The unexpected freeway closure offered an opportunistic change of plans. - Hazel Park, Michigan - July 2009
this is where printers used to assemble pages before a computerized pagination system was installed.
November 20: 39,000-odd people have come through here before me to this computerized test; my traits have been added to theirs.