Specifications - USS Artemis
Summary
General
Class | Akira-II Class | |
Registry | NCC 68241 | |
Role | Tactical Carrier | |
Commissioned | SD 236909.26 | |
Constructed | Begun SD236802.19, Antares Fleet Yards, Andoria | |
Finalized | Completed SD236907.13, Utopia Planitia Fleet Yards, Mars | |
Dedication | "The true test is in the trying, for it is in the trying that we find strength." -Unknown |
Dimensions
Length | 557.3m | |
Beam | 380m | |
Draft | 104.9m | |
Mass | 326,500 Metric Tonnes | |
Decks | 22 |
Personnel
Officers | 167 | |
Enlisted Crew | 356 | |
Marines | 41 |
Propulsion
Faster-Than-Light Drive | Class-IX FWY-4 M/ARA Reaction and Injection System | |
Maximum Warp Reactor Output | 61.6 Petawatts | |
Maximum Sustained Warp Stress Rating | 1640 Cochranes | |
Maximum Peak Warp Stress Rating | 2600 Cochranes | |
Cruise Speed | Warp 7.16 | |
Maximum Speed | Warp 9.17 | |
Emergency Speed | (36 Hrs Sustained) Warp 9.64 | |
Sublight Drive | Yoyodyne Propulsion Twin-Tandem Impulse Drive | |
Fusion Reactors | 2 Primary, 2 Secondary | |
Power Output | Primary Fusion Reactor: 7.8EJ/hr Secondary Fusion Reactor: 5.2EJ/hr |
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Maximum Impulse | 0.92c | |
Notes | The Akira-II Class warp field geometry is classified as 'forward-heavy', meaning that the ship's hull design and warp field allow it to sustain higher warp velocities with less power output from the warp drive than other similar mass starships. This allows the ship to cover greater distances with the same amount of fuel as other cruisers in the fleet. The drawback of this system is reduced maneuverability over conventional designs. |
Hull
External | Type-IV ablative armor | |
Central | Self-sealing tripolymer/duranium suspension | |
Internal | Tritanium/cortanium alloy |
Tactical & Defense
Phaser Systems | 6 Mk.VIII/20 Phaser Arrays: 1 fwd/port/dorsal 1 fwd/stbd/dorsal 1 aft/port/stbd/dorsal 1 fwd/port/stbd/ventral 1 fwd/port/aft/ventral 1 fwd/stbd/aft/ventral Maximum pD: 9.8 @ 0km 8.4 @ 70,000km 7.0 @ 150,000km Maximum Effective Range: 200,000km Maximum Emitter Energy Output: 5.6 Petajoules per second |
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Torpedo Systems | 3 Mk.IV Photon Torpedo Bays 2 Forward; 1 Aft Max Warhead Yield: 205 Petajoules (9.8 pD) Max Range at Max speed: 160,000km Max Range at Min speed: 81,920,000km Torpedo Loadout: 500 (150 Aft Launcher, 350 for two Fwd Launchers) |
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Defensive Measures | Shield Generator Type: FNSS70-90 Maximum Instantaneous Emitter Surge Load: 46.2 Petawatts Maximum Sustained Load: 52.2 Petawatts Advanced Features: Regenerative Adaptive Metaphasic Shielding Additional Measures: 18cm Ablative Armor |
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Notes | The Artemis is very lightly armed compared to other ships of her class, relying primarily on her fighter wing to provide defensive measures against hostile forces. In contrast, she has some of the best shields in the fleet backed by tough ablative armor. |
Flight Systems
Flight Bays | 1 Thru-deck Flight Operations Center | |
Auxiliary Shuttlebays | N/A | |
Shuttle /Starfighter Complement | Type 8 shuttlecraft: 3 Type 10 shuttlepods: 4 Danube-Class runabouts: 2 USS Palomino USS Freisian 36 Ranger Class Starfighters |
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Notes | Launch and recovery of Starfighter craft aboard an Akira is tricky business; launch itself is handled by guiding the craft out of the ship's Launch bay on a rail system, commonly referred to as a catapult. Four catapults are located on the main launch deck, though during normal day-to-day operations only two are used for fighter launches. In emergency scramble conditions, all four catapults are loaded with fighters and launched in ready sequence. |
Control & Scanning
Computer Specifications | Twin Bynaran 01-10 Bio-neural Tetralinear Computer Cores equipped with LCARS-4.2 interface matrix. Hardware/software design: Biolinear, Bio-neural geldisks Data transfer rate: 5.6 thousand kiloquads / second Primary storage capacity: 3.5 million kiloquads (per core) |
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Navigational Systems | Redundant high-power Navigational Deflectors Mk.11-A Proximity Array and Collision Warning System |
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Long Range Sensors | High resolution mode range: 14 light years (4.3 parsecs) Low resolution mode range: 30 light years (9.2 parsecs) Primary instruments: Wide-angle active EM scanner Variable frequency EM flux sensor Subspace field stress sensor Tachyon Detecting Spectrometer |
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Short Range Sensors | Effective Radius: 3 AU Primary instruments: Proximity sensor array type 11-A Lifeform analysis instrument cluster Thermal imaging array Gravimetric distortion scanner Passive neutrino imaging scanner Subspace differential pulse scanner Multiphasic scanner Magneton scanner Partical motion tracking sensors Weapons and Sensor targeting scanner |
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Science Instruments | Number of arrays: 12 Array compositions: 6 sensor pallet clusters per array Pallet 1: Wide-angle EM radiation imaging scanner Quark population analysis counter Z-range particulate spectrometry sensor Pallet 2: Active magnetic interferometry scanner High-energy proton spectrometry cluster Gravimetric distortion mapping scanner Isometric phase matrix imager Pallet 3: Pinpoint EM flux sensor ACB relay booster array Federation Timebase beacon receiver Stellar pair coordinate imager Pallet 4: Low-frequency EM flux sensor Localized subspace field stress sensor Parametric subspace field stress sensor Hydrogen-filter subspace flux scanner Linear calibration subspace flux sensor Pallet 5: Variable band optical imaging cluster Virtual aperture gravitron flux spectrometer High-resolution graviton flux spectrometer Very low energy graviton spin polarimeter Pallet 6: Active matrix gamma interferometry sensor Low-level thermal imaging sensor Multi-angle gamma frequency counter Virtual particle mapping camera Pallet 7: Quasar telescope Wide-angle IR Source Tracker Narrow-angle IR-UV-Gamma Ray Imager Active subspace multibeacon receiver Pallet 8: Stellar graviton detectors High-energy charged particle detectors Galactic plasma wave cartographic processor Impulse time-distortion corrector |
Environmental & Support
Communication Systems | Standard Communications Range: ~20 light years Standard Data Transmission Speed: 74 kq/s Subspace Communications Speed: Warp 9.9998 |
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Medical Facilities | 2 Intensive Care Wards 6 Stasis Units 4 Surgical Suites 1 Biohazard Isolation Unit 1 Null-Gravity Therapy Wards 1 Dental Office 1 Counseling Office |
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Recreational Facilities | 1 Large Holodecks 2 Holosuites 1 Gymnasium 1 Phaser Range 6 Cargo Bays 1 Recreation Room |
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Environmental Support | Able to sustain air and water for a maximum of 4500 people for 36 hours Air and Water system endurance 1,800 Sol years Food systems endurance with conservative replicator usage 1,660 Sol years Food systems endurance without replicators 66,300 Sol days Thermal capabilities -50 degrees C to +100 degrees C Artificial Gravity capabilities -3 to +7 Gs Inertial Dampeners capabilities +/- 82 billion Gs Inertial Dampener reaction time 0.014 attoseconds |
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Transporter System | Transporter Systems 2 Intensive Care Wards 6 Stasis Units 4 Surgical Suites 1 Biohazard Isolation Unit 1 Null-Gravity Therapy Wards 1 Dental Office 1 Counseling Office Personnel Transporters: Seven (6 person) Max Payload Mass / Pad: 900kg (1,763 lbs) Max Range: 40,000 km Beaming Rate: Approximately 1 person / pad / every 36 seconds Beaming Accuracy Rate: 99.99999% Emergency Transporters: Five (22 person) Max Range: 15,000km (send only - range dependent on available power) Max Beaming Rate: Approximately 1 person / pad / every 36 seconds Beaming Accuracy Rate: 99.99% Cargo Transporters: Two Max Payload Mass: 800 metric tons Max Payload Volume: 16 cubic meters Max Beaming Rate: Approximately once every 60 seconds Beaming Accuracy Rate: 99.97% |
Experimental Systems
LORASON-II | The LORASON (LOng-Range Astrometric/Sensor/Observation/Navigation) unit is a unique sensor suite, considered one of the greatest technological advancements in Starfleet sensor equipment to date. Equipped aboard Federation starships as a detachable pod unit, it provides high-resolution sensor data at ranges of up to 24 light-years, as well as a low-resolution range of up to 60 light-years - all dependant upon scanning parameters. Utilizing advanced Bio-Neural computing equipment, the LORASON unit processes sensor data in real time and is able to display it in its holographic Astrometrics center. The LORASON unit's processing abilities allow it to access all sensor platforms on a starship and combine the data into a single display. The LORASON-II unit is an upgrade that interfaces with the experimental DIRCOM subspace detection equipment presently installed aboard the USS Artemis. |
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DIRCOM | The DIRCOM (DIrection - Range - COMposition) system is a unique scanning tool recently developed by Starfleet R&D. The system basically operates by sending out warp field pulses over subspace. In Active mode, these pulses look for warp field signatures and resonances, and detect magnetic and polymer make-up when one is found. Though costly on power requirements and the necessity of a static warp field to use, the DIRCOM effectively plots warp-capable objects in subspace and normal space within a ten light-year radius. While in Active mode, DIRCOM scans are easily noticed, as they will 'ping' a ship's sensor systems, much like standard sensor systems. In Passive mode, the DIRCOM acts similar to a subspace communications antenna, 'listening' to the resonances of subspace within a five light-year radius. Less data is retrieved while in Passive mode, as the DIRCOM is only able to detect warp resonances in subspace and not in real space. Despite this, it is a great advantage in monitoring possible illegal traffic through less-guarded portions of the Federation's border. |