H-IIA 202 | Astro-H (Hitomi)

Launch information

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Mission description

Astro-H is the 6th satellite in a series of X-ray telescopes by JAXA and ISAS. Its 4 instruments on board will cover the X-ray and Gamma ray regions. This region consists of photons with energy ranging from 0.3-600keV, and the telescope will provide the highest resolution ever achieved of 3-10 keV bands. The craft weighs 2.7 tonnes and will be placed into a circular orbit 575km above the ground, with an inclination of 31 degrees.

Launch status

Launch status information for space mission ‘H-IIA 202 | Astro-H (Hitomi)’.

Launch image H-IIA 202 | Astro-H (Hitomi)

Success

Status: Launch Successful

Class: normal

Launch T0: Feb. 17, 2016, 8:45 a.m.

Timezone: Asia/Tokyo

Launch authority

Details about the the rocket, its target orbit and the launch pad location.

Mission

Astro-H (Hitomi) (LEO)

Launcher

Mitsubishi Heavy Industries

Rocket

H-IIA

Location

Tanegashima Space Center, Japan

Pad

Yoshinobu Launch Complex LP-1

Type

Astrophysics

Orbit

Low Earth Orbit (LEO)

Satellites on-board

Satellites on-board the space mission ‘H-IIA 202 | Astro-H (Hitomi)’ are identified by cross checking database entries for launches and satellites. Results could be inaccurate from time to time.

Number Name Orbit Inclination Country/Organization Status
41337 ASTRO H LEO 31.0 JAPAN In-orbit
41338 CHUBUSAT 2 LEO 31.0 JAPAN In-orbit
41339 CHUBUSAT 3 LEO 31.01 JAPAN In-orbit
41340 HORYU 4 LEO 31.0 JAPAN In-orbit

Launch statistics

Tracking key statistics for space mission ‘H-IIA 202 | Astro-H (Hitomi)’, classified in stats relative to the specific mission launch year or to all-time values.

Orbital Launch

#5531

To this date

Location Launch

#66

To this date

Pad Launch

#37

To this date

Agency Launch

#28

To this date

Orbital Launch

#12

Year 2016

Location Launch

#1

Year 2016

Pad Launch

#1

Year 2016

Agency Launch

#1

Year 2016

Latest news about the launch

No news available for this launch yet. Check back soon, we post updates daily.


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