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2. Native Command Queuing - Wikipedia

   en.wikipedia.org/wiki/Native_Command_Queuing

   NCQ allows the drive itself to determine the optimal order in which to retrieve outstanding requests. This may, as here, allow the drive to fulfill all requests in fewer rotations and thus less time. In computing , Native Command Queuing ( NCQ ) is an extension of the Serial ATA protocol allowing hard disk drives to internally optimize the ...

3. Seagate Technology - Wikipedia

   en.wikipedia.org/wiki/Seagate_Technology

   Back of a Seagate EXOS X18 18 TB HDD Seagate Barracuda HDD 160GB Model ST3160812AS Seagate Barracuda HDD 400GB Model ST3400820AS Seagate Barracuda Xt HDD 2TB Model ST32000641AS. Seagate offers various internal solid-state drive (SSD) and hard disk drive (HDD) products that are classed by name for their intended usage:

4. Seagate Barracuda - Wikipedia

   en.wikipedia.org/wiki/Seagate_Barracuda

   In 1993, Seagate released the first Barracuda drive, with the ST11950. The drive had a capacity of 2.03 GB (1.69 GB formatted), was available with FAST SCSI-2 (N/ND models) or WIDE SCSI-2 (W/WD models) interface, and was the first hard drive ever to have a spindle speed of 7200-RPM. Owing to the rotational speed, it was very fast but very ...

5. Hard disk drive interface - Wikipedia

   en.wikipedia.org/wiki/Hard_disk_drive_interface

   The drives within an A-unit and all other drives in a string had interfaces similar to the early interfaces, above. A-units connected to IBM Directors or integrated attachments . Small Computer System Interface (SCSI) , originally named SASI for Shugart Associates System Interface, is an early (circa 1978) industry standard interface explicitly ...

6. SyQuest Technology - Wikipedia

   en.wikipedia.org/wiki/SyQuest_Technology

   SyQuest Technology, Inc. (Nasdaq: SYQT) [1] was an early entrant into the hard disk drive market for personal computers.The company was founded on January 27, 1982 [2] by Syed Iftikar who had been a founder of Seagate, [3] along with Ben Alaimo, Bill Krajewski, Anil Nigam and George Toldi. [4]

7. K2-18b - Wikipedia

   en.wikipedia.org/wiki/K2-18b

   K2-18 is an M dwarf of the spectral class M3V [4] in the constellation Leo, [5] 38.025 ± 0.079 parsecs (124.02 ± 0.26 ly) away from the Sun. [1] The star is colder and smaller than the Sun, having a temperature of 3,457 K (3,184 °C; 5,763 °F) and a radius 45% of the Sun's, [6] and is not visible to the naked eye. [7]