The H-II Transfer Vehicle (HTV), also called Kounotori(こうのとり,Kōnotori, "Oriental stork" or "white stork"), is an automated cargo spacecraft used to resupply the Kibō Japanese Experiment Module (JEM) and the International Space Station (ISS). The Japan Aerospace Exploration Agency (JAXA) has been working on the design since the early 1990s. The first mission, HTV-1, was originally intended to be launched in 2001. It launched at 17:01 UTC on 10 September 2009 on an H-IIB launch vehicle. The name Kounotori was chosen for the HTV by JAXA because "a white stork carries an image of conveying an important thing (a baby, happiness, and other joyful things), therefore, it precisely expresses the HTV's mission to transport essential materials to the ISS". It is the vehicle of choice to complete the ACES program, a project designed to put two atomic clocks in space—on the ISS.
Design
The HTV is about 9.8m long (including maneuvering thrusters at one end) and 4.4m in diameter. Total mass is 10.5 tonnes, with a 6,000 kilograms (13,000lb) payload.
The HTV are comparable in function to the RussianProgress, EuropeanATV, commercial Dragon, and commercial Cygnus spacecraft, all of which bring or are planned to bring supplies to the ISS. Like the ATV, the HTV carries more than twice the payload of the Progress, but is launched less than half as often. Unlike Progress capsules and ATVs, which dock automatically, HTVs and American commercial spacecraft approach the ISS in stages, and are signaled by ISS crew or ground control to continue from one holding point to the next. Once they reach their closest parking orbit to the ISS, crew grapple them using the robotic arm Canadarm2 and berth them to an open berthing port on the Harmony module.
The H-II (H2) rocket was a Japanesesatellite launch system, which flew seven times between 1994 and 1999, with five successes. It was developed by NASDA in order to give Japan a capability to launch larger satellites in the 1990s. It was the first two-stage liquid-fuelled rocket Japan made using only technologies developed domestically. It was superseded by the H-IIA rocket following reliability and cost issues.
Background
Prior to H-II, NASDA had to use components licensed by the United States in its rockets. In particular, crucial technologies of the H-I and its predecessors were from the Delta rockets. The H-I did have domestically produced components, such as the LE-5 engine on the second stage and the inertial guidance system. H-II added to this by domestically developing the LE-7 liquid-fuel engine of the first stage and the solid booster rockets.
The H-II was developed under the following policies, according to a NASDA press release:
Develop the launch vehicle with Japanese space technology.
An HII region is a region of interstellar hydrogen that is ionized. It is typically a large, low-density cloud of partially ionized gas in which star formation has recently taken place. The short-lived blue stars forged in these regions emit copious amounts of ultraviolet light that ionize the surrounding gas. HII regions—sometimes several hundred light-years across—are often associated with giant molecular clouds. The first known HII region was the Orion Nebula, which was discovered in 1610 by Nicolas-Claude Fabri de Peiresc, although its nature was not known.
HII regions are named for the large amount of ionisedatomichydrogen they contain, referred to as HII, pronounced H-two by astronomers (an HI region being neutral atomic hydrogen, and a molecular cloud being molecular hydrogen, H2). Such regions have extremely diverse shapes, because the distribution of the stars and gas inside them is irregular. They often appear clumpy and filamentary, sometimes showing bizarre shapes such as the Horsehead Nebula. HII regions may give birth to thousands of stars over a period of several million years. In the end, supernova explosions and strong stellar winds from the most massive stars in the resulting star cluster will disperse the gases of the HII region, leaving behind a cluster of birthed stars such as the Pleiades.
Stars are born off of collapsing gas clouds due to gravity. Owing to intense high energy UV radiation of the newly formed stars, the surrounding gas cloud gets ionized. This region of ionized atomic hydrogen is known as an H II region.
‘H II’ (pronounced as H-2) represents singly ionized hydrogen atom. In astronomy, neutral atoms are represented by their atomic symbols followed by I. While the charged species are followed by II, III and so on. For instance,
Neutral Hydrogen (H) - H I,
Singly Ionized Hydrogen (H+) - H II,
Neutral Oxygen (O) - O I,
Doubly Ionized Oxygen (O2+) - O III.
Such regions usually span from one to hundreds of light years, having temperatures around 10,000 K. H II regions give birth to thousands of short-lived blue star clusters, which radiate copious amounts of lig...
published: 27 Jan 2021
Astronomy - Ch. 28: The Milky Way (18 of 27) H II (Hydrogen II) Regions
Visit http://ilectureonline.com for more math and science lectures!
To donate:
http://www.ilectureonline.com/donate
https://www.patreon.com/user?u=3236071
We will learn H II regions are regions containing ionized hydrogen gas such as emission nebulae which have bright stars embedded within them that produce UV radiation.
1) exists mostly within the spirals
2) highest concentration about 10,000 l.y. From the galactic center
3) observed using radio astronomy
and more...
Next video in this series can be seen at:
https://youtu.be/kZpeZuzil_A
published: 26 May 2020
Zooming in on the HII Region LHA 120-N 180B
This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a dazzling region of newly-forming stars in the HII region LHA 120-N 180B — also known as N180. This glowing region of newborn stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
More information and download options: http://www.eso.org/public/videos/eso1903b/
Credit:
ESO/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral Electronic
published: 06 Feb 2019
Hii
Hii again
published: 22 Jun 2022
HII Regions and Star Forming Regions
The Interstellar Medium is laced with Star Forming Regions. These comprise some of the most wonderful locations in the sky. The Eagle Nebula, the Trifid Nebula, and others are great examples. H-II regions are very pretty to see in the sky, but they also are the places where stars are created. This is part of my complete intro Astronomy class that I taught at Willam Paterson University and CUNY Hunter.
0:00 Introduction
0:01 The Interstellar Medium
0:52 The Three Phases of the ISM
5:13 Nebular Properties
12:19 Star-Forming Regions
14:55 How nebulae make the light we see
20:54 Baby Stars in the Trifid Nebula
Supplement the videos with "OpenStax Astronomy"
https://openstax.org/books/astronomy/pages/20-thinking-ahead
20: Between the Stars: Gas and Dust in Space
https://openstax.org/boo...
published: 24 Aug 2018
HII Benefits
Looking for a great place to work with benefits that are second to none? Look no further than HII. And for those of you already on board, HII’s benefits are with you on your wellness journey!
published: 16 May 2022
o no no 😂 #shorts #viral #funny #comedy @ateetkxyz
Stars are born off of collapsing gas clouds due to gravity. Owing to intense high energy UV radiation of the newly formed stars, the surrounding gas cloud gets ...
Stars are born off of collapsing gas clouds due to gravity. Owing to intense high energy UV radiation of the newly formed stars, the surrounding gas cloud gets ionized. This region of ionized atomic hydrogen is known as an H II region.
‘H II’ (pronounced as H-2) represents singly ionized hydrogen atom. In astronomy, neutral atoms are represented by their atomic symbols followed by I. While the charged species are followed by II, III and so on. For instance,
Neutral Hydrogen (H) - H I,
Singly Ionized Hydrogen (H+) - H II,
Neutral Oxygen (O) - O I,
Doubly Ionized Oxygen (O2+) - O III.
Such regions usually span from one to hundreds of light years, having temperatures around 10,000 K. H II regions give birth to thousands of short-lived blue star clusters, which radiate copious amounts of light - illuminating the nebula. Owing to strong stellar winds, radiation pressure and supernova explosions, such regions get dispersed within a few million years of star formation event.
PLEIADES
Pleiades is one such star cluster, where the surrounding H II region is getting dispersed due to the strong stellar winds of B-type stars.
ORION NEBULA
Another famous example is the Orion Nebula, where the stars of the Trapezium Cluster are ionizing the cloud. The Orion Nebula (M42), located 500 pc away, is a part of the Orion Molecular Cloud Complex.
HORSEHEAD NEBULA
Horsehead Nebula is another active star forming H II region in the Orion Molecular Cloud Complex. Presence of thick dust in front of the stars results in the extinguishing of light. The silhouette of the dark nebula visible against the complex and intricate structure is absolutely breathtaking.
H II regions comprise mostly 90% hydrogen, some helium and traces of other heavy elements. The strongest hydrogen emission line, the H-alpha line at 656.3 nm, gives H II regions their characteristic red colour.
H II regions are mostly found in the arms of spiral galaxies and throughout irregular galaxies.
TARANTULA NEBULA
Tarantula Nebula is the most massive H II region - 2nd largest in the Local Group of Galaxies. It is located 160 kly away in the LMC (a satellite galaxy of Milky Way). Thousands of OB and Wolf-Rayet stars populate this region. In fact, the most massive star known - R136a1 (215 M☉) - is located in the central concentration of this region.
NGC 604
NGC 604 is the largest H II region in the entire Local Group of Galaxies, spanning 1,520 ly in diameter. This H II region is located in the Triangulum Galaxy, 2.7 million ly away.
The young stars in H II regions show evidence for containing planetary systems. The Hubble Space Telescope has revealed hundreds of protoplanetary disks (proplyds) in the Orion Nebula.
______________________________________________________________
Graphics: NASA, ESA, ESO, Space Engine
Music: Aiur Oscar - Island Syllan
https://www.youtube.com/watch?v=iFwLjRaxI5Q
❚ Aiur Oscar
• https://soundcloud.com/aiuroscar
• https://facebook.com/AiurOscar/
• https://www.youtube.com/channel/UCbuypWF9W0FIvg3NG6C5g3Q
______________________________________________________________
SUBSCRIBE
celeris
Stars are born off of collapsing gas clouds due to gravity. Owing to intense high energy UV radiation of the newly formed stars, the surrounding gas cloud gets ionized. This region of ionized atomic hydrogen is known as an H II region.
‘H II’ (pronounced as H-2) represents singly ionized hydrogen atom. In astronomy, neutral atoms are represented by their atomic symbols followed by I. While the charged species are followed by II, III and so on. For instance,
Neutral Hydrogen (H) - H I,
Singly Ionized Hydrogen (H+) - H II,
Neutral Oxygen (O) - O I,
Doubly Ionized Oxygen (O2+) - O III.
Such regions usually span from one to hundreds of light years, having temperatures around 10,000 K. H II regions give birth to thousands of short-lived blue star clusters, which radiate copious amounts of light - illuminating the nebula. Owing to strong stellar winds, radiation pressure and supernova explosions, such regions get dispersed within a few million years of star formation event.
PLEIADES
Pleiades is one such star cluster, where the surrounding H II region is getting dispersed due to the strong stellar winds of B-type stars.
ORION NEBULA
Another famous example is the Orion Nebula, where the stars of the Trapezium Cluster are ionizing the cloud. The Orion Nebula (M42), located 500 pc away, is a part of the Orion Molecular Cloud Complex.
HORSEHEAD NEBULA
Horsehead Nebula is another active star forming H II region in the Orion Molecular Cloud Complex. Presence of thick dust in front of the stars results in the extinguishing of light. The silhouette of the dark nebula visible against the complex and intricate structure is absolutely breathtaking.
H II regions comprise mostly 90% hydrogen, some helium and traces of other heavy elements. The strongest hydrogen emission line, the H-alpha line at 656.3 nm, gives H II regions their characteristic red colour.
H II regions are mostly found in the arms of spiral galaxies and throughout irregular galaxies.
TARANTULA NEBULA
Tarantula Nebula is the most massive H II region - 2nd largest in the Local Group of Galaxies. It is located 160 kly away in the LMC (a satellite galaxy of Milky Way). Thousands of OB and Wolf-Rayet stars populate this region. In fact, the most massive star known - R136a1 (215 M☉) - is located in the central concentration of this region.
NGC 604
NGC 604 is the largest H II region in the entire Local Group of Galaxies, spanning 1,520 ly in diameter. This H II region is located in the Triangulum Galaxy, 2.7 million ly away.
The young stars in H II regions show evidence for containing planetary systems. The Hubble Space Telescope has revealed hundreds of protoplanetary disks (proplyds) in the Orion Nebula.
______________________________________________________________
Graphics: NASA, ESA, ESO, Space Engine
Music: Aiur Oscar - Island Syllan
https://www.youtube.com/watch?v=iFwLjRaxI5Q
❚ Aiur Oscar
• https://soundcloud.com/aiuroscar
• https://facebook.com/AiurOscar/
• https://www.youtube.com/channel/UCbuypWF9W0FIvg3NG6C5g3Q
______________________________________________________________
SUBSCRIBE
celeris
Visit http://ilectureonline.com for more math and science lectures!
To donate:
http://www.ilectureonline.com/donate
https://www.patreon.com/user?u=3236071
We ...
Visit http://ilectureonline.com for more math and science lectures!
To donate:
http://www.ilectureonline.com/donate
https://www.patreon.com/user?u=3236071
We will learn H II regions are regions containing ionized hydrogen gas such as emission nebulae which have bright stars embedded within them that produce UV radiation.
1) exists mostly within the spirals
2) highest concentration about 10,000 l.y. From the galactic center
3) observed using radio astronomy
and more...
Next video in this series can be seen at:
https://youtu.be/kZpeZuzil_A
Visit http://ilectureonline.com for more math and science lectures!
To donate:
http://www.ilectureonline.com/donate
https://www.patreon.com/user?u=3236071
We will learn H II regions are regions containing ionized hydrogen gas such as emission nebulae which have bright stars embedded within them that produce UV radiation.
1) exists mostly within the spirals
2) highest concentration about 10,000 l.y. From the galactic center
3) observed using radio astronomy
and more...
Next video in this series can be seen at:
https://youtu.be/kZpeZuzil_A
This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a dazzling region of newly-forming stars in the HII region LHA 120-N 1...
This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a dazzling region of newly-forming stars in the HII region LHA 120-N 180B — also known as N180. This glowing region of newborn stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
More information and download options: http://www.eso.org/public/videos/eso1903b/
Credit:
ESO/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral Electronic
This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a dazzling region of newly-forming stars in the HII region LHA 120-N 180B — also known as N180. This glowing region of newborn stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
More information and download options: http://www.eso.org/public/videos/eso1903b/
Credit:
ESO/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral Electronic
The Interstellar Medium is laced with Star Forming Regions. These comprise some of the most wonderful locations in the sky. The Eagle Nebula, the Trifid Nebul...
The Interstellar Medium is laced with Star Forming Regions. These comprise some of the most wonderful locations in the sky. The Eagle Nebula, the Trifid Nebula, and others are great examples. H-II regions are very pretty to see in the sky, but they also are the places where stars are created. This is part of my complete intro Astronomy class that I taught at Willam Paterson University and CUNY Hunter.
0:00 Introduction
0:01 The Interstellar Medium
0:52 The Three Phases of the ISM
5:13 Nebular Properties
12:19 Star-Forming Regions
14:55 How nebulae make the light we see
20:54 Baby Stars in the Trifid Nebula
Supplement the videos with "OpenStax Astronomy"
https://openstax.org/books/astronomy/pages/20-thinking-ahead
20: Between the Stars: Gas and Dust in Space
https://openstax.org/books/astronomy/pages/21-thinking-ahead
21: The Birth of Stars and the Discovery of Planets outside the Solar System
https://en.wikipedia.org/wiki/Interstellar_medium
Interstellar Medium
https://en.wikipedia.org/wiki/Star_formation#Stellar_nurseries
Star Forming Regions
https://en.wikipedia.org/wiki/H_II_region
H-II region
https://en.wikipedia.org/wiki/Eagle_Nebula
Eagle Nebula
https://en.wikipedia.org/wiki/Trifid_Nebula
Trifid Nebula
https://en.wikipedia.org/wiki/Str%C3%B6mgren_sphere
Strömgren sphere
http://astro-cabinet.com/about.php
Dieter Willasch's AstroCabinet
The Interstellar Medium is laced with Star Forming Regions. These comprise some of the most wonderful locations in the sky. The Eagle Nebula, the Trifid Nebula, and others are great examples. H-II regions are very pretty to see in the sky, but they also are the places where stars are created. This is part of my complete intro Astronomy class that I taught at Willam Paterson University and CUNY Hunter.
0:00 Introduction
0:01 The Interstellar Medium
0:52 The Three Phases of the ISM
5:13 Nebular Properties
12:19 Star-Forming Regions
14:55 How nebulae make the light we see
20:54 Baby Stars in the Trifid Nebula
Supplement the videos with "OpenStax Astronomy"
https://openstax.org/books/astronomy/pages/20-thinking-ahead
20: Between the Stars: Gas and Dust in Space
https://openstax.org/books/astronomy/pages/21-thinking-ahead
21: The Birth of Stars and the Discovery of Planets outside the Solar System
https://en.wikipedia.org/wiki/Interstellar_medium
Interstellar Medium
https://en.wikipedia.org/wiki/Star_formation#Stellar_nurseries
Star Forming Regions
https://en.wikipedia.org/wiki/H_II_region
H-II region
https://en.wikipedia.org/wiki/Eagle_Nebula
Eagle Nebula
https://en.wikipedia.org/wiki/Trifid_Nebula
Trifid Nebula
https://en.wikipedia.org/wiki/Str%C3%B6mgren_sphere
Strömgren sphere
http://astro-cabinet.com/about.php
Dieter Willasch's AstroCabinet
Looking for a great place to work with benefits that are second to none? Look no further than HII. And for those of you already on board, HII’s benefits are wit...
Looking for a great place to work with benefits that are second to none? Look no further than HII. And for those of you already on board, HII’s benefits are with you on your wellness journey!
Looking for a great place to work with benefits that are second to none? Look no further than HII. And for those of you already on board, HII’s benefits are with you on your wellness journey!
Stars are born off of collapsing gas clouds due to gravity. Owing to intense high energy UV radiation of the newly formed stars, the surrounding gas cloud gets ionized. This region of ionized atomic hydrogen is known as an H II region.
‘H II’ (pronounced as H-2) represents singly ionized hydrogen atom. In astronomy, neutral atoms are represented by their atomic symbols followed by I. While the charged species are followed by II, III and so on. For instance,
Neutral Hydrogen (H) - H I,
Singly Ionized Hydrogen (H+) - H II,
Neutral Oxygen (O) - O I,
Doubly Ionized Oxygen (O2+) - O III.
Such regions usually span from one to hundreds of light years, having temperatures around 10,000 K. H II regions give birth to thousands of short-lived blue star clusters, which radiate copious amounts of light - illuminating the nebula. Owing to strong stellar winds, radiation pressure and supernova explosions, such regions get dispersed within a few million years of star formation event.
PLEIADES
Pleiades is one such star cluster, where the surrounding H II region is getting dispersed due to the strong stellar winds of B-type stars.
ORION NEBULA
Another famous example is the Orion Nebula, where the stars of the Trapezium Cluster are ionizing the cloud. The Orion Nebula (M42), located 500 pc away, is a part of the Orion Molecular Cloud Complex.
HORSEHEAD NEBULA
Horsehead Nebula is another active star forming H II region in the Orion Molecular Cloud Complex. Presence of thick dust in front of the stars results in the extinguishing of light. The silhouette of the dark nebula visible against the complex and intricate structure is absolutely breathtaking.
H II regions comprise mostly 90% hydrogen, some helium and traces of other heavy elements. The strongest hydrogen emission line, the H-alpha line at 656.3 nm, gives H II regions their characteristic red colour.
H II regions are mostly found in the arms of spiral galaxies and throughout irregular galaxies.
TARANTULA NEBULA
Tarantula Nebula is the most massive H II region - 2nd largest in the Local Group of Galaxies. It is located 160 kly away in the LMC (a satellite galaxy of Milky Way). Thousands of OB and Wolf-Rayet stars populate this region. In fact, the most massive star known - R136a1 (215 M☉) - is located in the central concentration of this region.
NGC 604
NGC 604 is the largest H II region in the entire Local Group of Galaxies, spanning 1,520 ly in diameter. This H II region is located in the Triangulum Galaxy, 2.7 million ly away.
The young stars in H II regions show evidence for containing planetary systems. The Hubble Space Telescope has revealed hundreds of protoplanetary disks (proplyds) in the Orion Nebula.
______________________________________________________________
Graphics: NASA, ESA, ESO, Space Engine
Music: Aiur Oscar - Island Syllan
https://www.youtube.com/watch?v=iFwLjRaxI5Q
❚ Aiur Oscar
• https://soundcloud.com/aiuroscar
• https://facebook.com/AiurOscar/
• https://www.youtube.com/channel/UCbuypWF9W0FIvg3NG6C5g3Q
______________________________________________________________
SUBSCRIBE
celeris
Visit http://ilectureonline.com for more math and science lectures!
To donate:
http://www.ilectureonline.com/donate
https://www.patreon.com/user?u=3236071
We will learn H II regions are regions containing ionized hydrogen gas such as emission nebulae which have bright stars embedded within them that produce UV radiation.
1) exists mostly within the spirals
2) highest concentration about 10,000 l.y. From the galactic center
3) observed using radio astronomy
and more...
Next video in this series can be seen at:
https://youtu.be/kZpeZuzil_A
This zoom video starts with a wide view of the Milky Way and ends with a close-up look at a dazzling region of newly-forming stars in the HII region LHA 120-N 180B — also known as N180. This glowing region of newborn stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
More information and download options: http://www.eso.org/public/videos/eso1903b/
Credit:
ESO/Digitized Sky Survey 2/N. Risinger (skysurvey.org). Music: Astral Electronic
The Interstellar Medium is laced with Star Forming Regions. These comprise some of the most wonderful locations in the sky. The Eagle Nebula, the Trifid Nebula, and others are great examples. H-II regions are very pretty to see in the sky, but they also are the places where stars are created. This is part of my complete intro Astronomy class that I taught at Willam Paterson University and CUNY Hunter.
0:00 Introduction
0:01 The Interstellar Medium
0:52 The Three Phases of the ISM
5:13 Nebular Properties
12:19 Star-Forming Regions
14:55 How nebulae make the light we see
20:54 Baby Stars in the Trifid Nebula
Supplement the videos with "OpenStax Astronomy"
https://openstax.org/books/astronomy/pages/20-thinking-ahead
20: Between the Stars: Gas and Dust in Space
https://openstax.org/books/astronomy/pages/21-thinking-ahead
21: The Birth of Stars and the Discovery of Planets outside the Solar System
https://en.wikipedia.org/wiki/Interstellar_medium
Interstellar Medium
https://en.wikipedia.org/wiki/Star_formation#Stellar_nurseries
Star Forming Regions
https://en.wikipedia.org/wiki/H_II_region
H-II region
https://en.wikipedia.org/wiki/Eagle_Nebula
Eagle Nebula
https://en.wikipedia.org/wiki/Trifid_Nebula
Trifid Nebula
https://en.wikipedia.org/wiki/Str%C3%B6mgren_sphere
Strömgren sphere
http://astro-cabinet.com/about.php
Dieter Willasch's AstroCabinet
Looking for a great place to work with benefits that are second to none? Look no further than HII. And for those of you already on board, HII’s benefits are with you on your wellness journey!
The H-II Transfer Vehicle (HTV), also called Kounotori(こうのとり,Kōnotori, "Oriental stork" or "white stork"), is an automated cargo spacecraft used to resupply the Kibō Japanese Experiment Module (JEM) and the International Space Station (ISS). The Japan Aerospace Exploration Agency (JAXA) has been working on the design since the early 1990s. The first mission, HTV-1, was originally intended to be launched in 2001. It launched at 17:01 UTC on 10 September 2009 on an H-IIB launch vehicle. The name Kounotori was chosen for the HTV by JAXA because "a white stork carries an image of conveying an important thing (a baby, happiness, and other joyful things), therefore, it precisely expresses the HTV's mission to transport essential materials to the ISS". It is the vehicle of choice to complete the ACES program, a project designed to put two atomic clocks in space—on the ISS.
Design
The HTV is about 9.8m long (including maneuvering thrusters at one end) and 4.4m in diameter. Total mass is 10.5 tonnes, with a 6,000 kilograms (13,000lb) payload.
The HTV are comparable in function to the RussianProgress, EuropeanATV, commercial Dragon, and commercial Cygnus spacecraft, all of which bring or are planned to bring supplies to the ISS. Like the ATV, the HTV carries more than twice the payload of the Progress, but is launched less than half as often. Unlike Progress capsules and ATVs, which dock automatically, HTVs and American commercial spacecraft approach the ISS in stages, and are signaled by ISS crew or ground control to continue from one holding point to the next. Once they reach their closest parking orbit to the ISS, crew grapple them using the robotic arm Canadarm2 and berth them to an open berthing port on the Harmony module.
Verse 1: I specialize in poetic calisthenics And stay on my P's and Q's like alphabetics Who else could it be but no other then the P.R.O.B. L.E.M.Z. and my right hand man from G.P. B.K. collaboration we spark lye stay high like inflation (What?) Patient back and fourth on this track Puttin' facts on wax without hesitation They'll be no mistakin' we makin' Nothin' but power moves I'll representation While DJ Honda cut shit up like Jason Cross fadin' back and forth on S.L. Twelve double 0 spark dros get blessed L's Get twisted like pretzels when the dred sells Me the buddah blessed I spark up then the red cells In my eyes become highly prevalent, anti benevolent Never hesitant to represent Hook: Fromt he land of G.P. to the streets of F.B. "I represent from midnight to high noon" -GZA 'Liquid Swords' Problemz Honda collaboration been awaitin' From the streets of F.B. to the land of G.P. "I represent from midnight to high noon" "Drop megaton bombs" -GZA 'Liquid Swords' Verse 2: A-yo this industry is overflooded with acresses and actors Perpetrating the role of rappers with theatric tactics Constantly contributing to wackness Never surpass this cause you lack this perhaps it's Your lack of practice got you soundin' ass backwards Well I'm here to flip the script like gymnastics On y'all wack bastards The shit I kick is from the heart rappers use to rhymes now there's nothing but actors playin' parts Instead of spendin' time in the lab writtin' lines Niggas is basin' they whole rhyme on fictonal crime When half the time These niggas is straight up suburbaners Talkin' about they murderers and burgulars Hook Verse 3: A-yo I manufacture hits like a factory my faculty Is backin' rappin' be what enables me To live lavishly Happily ever after who the master Rememver me Problemz comprehending me? Mad energy when it be time for action No swingin' or knuckles strickly ammo blastin' Kill The Noise part II J.P., P.K. collaboration to be continuned Hook
To facilitate the pooling of funds, all capital was transferred to a special purpose vehicle (SPV) dubbed OpenAI Startup Fund SPV II, L.P ... A few weeks ago, Altman took the bold step of transferring ...
The Columbus Telegram
05 Jul 2023
The Columbus Telegram
05 Jul 2023