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NTC008HP00- NTC SENSOR IP67 -50T50 (-50T100 ON AIR) 0.8 METER LONG
The precision reached thanks to the technical solutions adopted in the development of these sensors and the reliability proven by the tests performed make CAREL NTC probes reliable and affordable transducers for measuring temperature.
The range of CAREL temperature sensors now includes TS* series (with two new immersion sensors, NTC and PT1000, suitable exclusively for hydronic applications) and a new pass-through temperature sensor to be used in the blast chiller applications, where the sensor is used for measuring the temperature in the product heart.
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Picnic Young | LABS 2008.
Sensor Machines
Zou het niet gaaf zijn als de muziek vanzelf reageert op jouw bewegingen? Je zou bijvoorbeeld een dansmat kunnen maken die het soort muziek aanpast op hoe jij danst. Of wat dacht je van 'magic drum sticks': als jij bewegingen met je stokjes in de lucht maakt, vul je de ruimte met een
drumsolo. Leerlingen maken in dit Lab een interactieve muziekinstallatie, waarmee ze aan het eind van de workshop een optreden geven.
Het ingraveren van eigen naam op eigen mobiel is erg populair.
Sensor from optic unit for CD-ROM player. Original size is about 1x1 mm.
First ever attempt way back in 2007.
This is the 5D MarkIII with the Tokina AT-X 116 11-16mm f2.8 at 11mm. It's what happens when you use it on a camera with a full-frame sensor.
21 April 2024, 01:32 UT; Stuart, Florida USA.
Celestron 200mm SCT at f/6. QHY 294M Pro camera, bin 2, exposure 15s, Mono16, gain 1600, stack of 104 frames, Optolong UHC filter, no guiding, no calibration frames, sensor -10°C. Processed in Pixinsight and Photoshop.
Appearance: Small face-on spiral galaxy with a bright center, knotty texture, and suggestion of three poorly resolved spiral arms.
Clouds: partly cloudy
Transparency: below average
Seeing: below average
Magnitude: 11.3
Apparent size: 1.7 x 1.4 arcmin
Moon age, illuminated: 12d, 93%
Azimuth 11°
Altitude 54°
from Wikipedia
Type: SA(rs)bc
NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated 70 million light years from the Sun. The morphological classification of SA(rs)bc indicates this is a spiral galaxy the lacks a bar; the 'rs' means it has a weakly-formed ring structure, and the 'bc' indicates the spiral arms are moderately to loosely wound.
The galaxy is inclined by around 20° to the line of sight from the Earth. It is forming new stars at the estimated rate of 4.10 M☉ yr−1, which is fairly typical for a galaxy of this morphology. The star formation rate is much higher in the central region, which may be the result of recent merger with a dwarf galaxy within the last 100 million years.
This galaxy has no detected activity in the nuclear region. There is a rotating nuclear disk of high brightness at the core that is consistent with the presence of a compact mass of 1×10^7 M☉. Most likely this is a supermassive black hole (SMBH).
On July 29, 1994, the type IIp supernova designated SN 1994W was discovered in this galaxy by Giancarlo Cortini and Mirko Villi. The event reached peak visual magnitude on August 13, and declined thereafter. It was located about 19 arc seconds to the northwest of the nucleus. This supernova was unusual for the exceptionally low quantity of nickel-56 released—indeed, it was the lowest inferred amount measured for any type II supernova as of that date. Based upon a possible detection of X-ray emission from the remnant, this may be a high-luminosity type IIn supernova.
NGC 4041 is a member of the LGG 266 galaxy group, along with NGC 4036, IC 758, UGC 7009, and UGC 7019. It is located just 17 arc minutes from NGC 4036, and the two form a pair with a projected separation of around 470 kly (143 kpc).
Again, hard to see but this is the sensor wire going under the fuse box to the hole for the ABS sensor.
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