My Weigh T3 400 Triton T3 400 Gram x 0.01 Digital Pocket Scale Black

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The orbital properties of Triton were already determined with high accuracy in the 19th century. It was found to have a retrograde orbit, at a very high angle of inclination to the plane of Neptune's orbit. The first detailed observations of Triton were not made until 1930. Little was known about the satellite until Voyager 2 flew by in 1989. [7]

My Weigh Triton T3-R Rechargeable Pocket Scale | 500g x 0.01g

One of the largest cryovolcanic features found on Triton is Leviathan Patera, [57] a caldera-like feature roughly 100km in diameter seen near the equator. Surrounding this caldera is a volcanic dome that stretches for roughly 2,000km along its longest axis, indicating that Leviathan is the second largest volcano in the solar system by area, after Alba Mons. This feature is also connected to two enormous cryolava lakes seen northwest of the caldera. Because the cryolava on Triton is believed to be primarily water ice with some ammonia, these lakes would qualify as stable bodies of surface liquid water while they were molten. This is the first place such bodies have been found apart from Earth, and Triton is the only icy body known to feature cryolava lakes, although similar cryomagmatic extrusions can be seen on Ariel, Ganymede, Charon, and Titan. [58] In the second bar of the example, you can see these notes divided into two major triads, one from the root and one from the tritone note (Gb in this case).As you can see, the C7b9#11 chord has the notes C E F#(Gb) Bb and Db. There is also a G in this chord, but we don’t usually have enough fingers to play it, so it gets left out. Triton was discovered by British astronomer William Lassell on October 10, 1846, [17] just 17days after the discovery of Neptune. When John Herschel received news of Neptune's discovery, he wrote to Lassell suggesting he search for possible moons. Lassell discovered Triton eight days later. [17] [18] Lassell also claimed for a period [h] to have discovered rings. [19] Although Neptune was later confirmed to have rings, they are so faint and dark that it is not plausible he saw them. A brewer by trade, Lassell spotted Triton with his self-built 61cm (24in) aperture metal mirror reflecting telescope (also known as the "two-foot" reflector). [20] This telescope was donated to the Royal Observatory, Greenwich in the 1880s, but was eventually dismantled. [20]

Triton at Scale with MIG and Kubernetes Deploying NVIDIA Triton at Scale with MIG and Kubernetes

Polar cap, plains and ridges [ edit ] Triton's bright south polar cap above a region of cantaloupe terrain The tritone scale has the intervals, Root-b2-3-b5-5-b7, so all of those juicy notes we saw in the C7b9#11 chord in the first bar of the example. Now that you know how to build a tritone scale, R-b2-3-b5-5-b7, let’s take a look at a few common fingerings for this scale on the guitar. Triton has a tenuous nitrogen atmosphere, with trace amounts of carbon monoxide and small amounts of methane near its surface. [11] [42] [43] Like Pluto's atmosphere, the atmosphere of Triton is thought to have resulted from the evaporation of nitrogen from its surface. [27] Its surface temperature is at least 35.6K (−237.6°C) because Triton's nitrogen ice is in the warmer, hexagonal crystalline state, and the phase transition between hexagonal and cubic nitrogen ice occurs at that temperature. [44] An upper limit in the low 40s (K) can be set from vapor pressure equilibrium with nitrogen gas in Triton's atmosphere. [45] This is colder than Pluto's average equilibrium temperature of 44K (−229.2°C). Triton's surface atmospheric pressure is only about 1.4–1.9 Pa (0.014–0.019 mbar). [7] Clouds observed above Triton's limb by Voyager 2. There are a number of ways to play the tritone scale on the guitar, but here are two of my favorites.Because of this relationship, between the tritone scale and the 7b9#11 chord, the tritone scale is often used over a 7alt chord to produce the b9 and #11 alterations, or over a dominant 7th chord where you want to create tension you can later resolve over the same chord, or over the next chord in the progression. Cantaloupe terrain, which is mostly dirty water ice, is only known to exist on Triton. It contains depressions 30–40km in diameter. [68] The depressions ( cavi) are probably not impact craters because they are all of the similar size and have smooth curves. The leading hypothesis for their formation is diapirism, the rising of "lumps" of less dense material through a stratum of denser material. [7] [69] Alternative hypotheses include formation by collapses, or by flooding caused by cryovolcanism. [68] Impact craters [ edit ] Tuonela Planitia (left) and Ruach Planitia (center) are two of Triton's cryovolcanic "walled plains". The paucity of craters is evidence of extensive, relatively recent, geologic activity. In 1997, observations from Earth were made of Triton's limb as it passed in front of stars. These observations indicated the presence of a denser atmosphere than was deduced from Voyager 2 data. [48] Other observations have shown an increase in temperature by 5% from 1989 to 1998. [49] These observations indicated Triton was approaching an unusually warm southern hemisphere summer season that happens only once every few hundred years. Theories for this warming include a change of frost patterns on Triton's surface and a change in ice albedo, which would allow more heat to be absorbed. [50] Another theory argues that temperature changes are a result of the deposition of dark, red material from geological processes. Because Triton's Bond albedo is among the highest in the Solar System, it is sensitive to small variations in spectral albedo. [51] Surface features [ edit ] Interpretative geomorphological map of Triton

was it nicknamed the devil’s What is a tritone and why was it nicknamed the devil’s

The few impact craters on Triton are almost all concentrated in the leading hemisphere—that facing the direction of the orbital motion—with the majority concentrated around the equator between 30° and 70° longitude, [70] resulting from material swept up from orbit around Neptune. [54] Because it orbits with one side permanently facing the planet, astronomers expect that Triton should have fewer impacts on its trailing hemisphere, due to impacts on the leading hemisphere being more frequent and more violent. [70] Voyager 2 imaged only 40% of Triton's surface, so this remains uncertain. However, the observed cratering asymmetry exceeds what can be explained based on the impactor populations, and implies a younger surface age for the crater-free regions (≤ 6million years old) than for the cratered regions (≤ 50million years old). [53] Observation and exploration [ edit ] NASA illustration detailing the studies of the proposed Trident mission Neptune (top) and Triton (bottom) three days after flyby of Voyager 2 Triton is the seventh-largest moon and sixteenth-largest object in the Solar System and is modestly larger than the dwarf planets Pluto and Eris. It is also the largest retrograde moon in the solar system. It comprises more than 99.5% of all the mass known to orbit Neptune, including the planet's rings and thirteen other known moons, [j] and is also more massive than all known moons in the Solar System smaller than itself combined. [k] Also, with a diameter 5.5% that of Neptune, it is the largest moon of a gas giant relative to its planet in terms of diameter, although Titan is bigger relative to Saturn in terms of mass (the ratio of Triton's mass to that of Neptune is approximately 1:4788). It has a radius, density (2.061 g/cm 3), temperature and chemical composition similar to that of Pluto. [33] Play a ii V I in the key of C major and use the tritone scale to build your solo lines over the V7 chord in that progression. Repeat in 12 keysTriton's western hemisphere consists of a strange series of fissures and depressions known as "cantaloupe terrain" because it resembles the skin of a cantaloupe melon. Although it has few craters, it is thought that this is the oldest terrain on Triton. [68] It probably covers much of Triton's western half. [7] Triton's orbit is associated with two tilts, the obliquity of Neptune's rotation to Neptune's orbit, 30°, and the inclination of Triton's orbit to Neptune's rotation, 157° (an inclination over 90° indicates retrograde motion). Triton's orbit precesses forward relative to Neptune's rotation with a period of about 678 Earth years (4.1 Neptunian years), [4] [5] making its Neptune-orbit-relative inclination vary between 127° and 173°. That inclination is currently 130°; Triton's orbit is now near its maximum departure from coplanarity with Neptune's. The Voyager 2 probe in 1989 observed a handful of geyser-like eruptions of nitrogen gas and entrained dust from beneath the surface of Triton in plumes up to 8km high. [33] [59] Triton is thus, along with Earth, Io, Europa and Enceladus, one of the few bodies in the Solar System on which active eruptions of some sort have been observed. [60] The best-observed examples are named Hili and Mahilani (after a Zulu water sprite and a Tongan sea spirit, respectively). [61]