Astronaut Janice Voss KC5BTK – SK

Astronaut Janice Voss KC5BTK - SK

Astronaut Janice Voss KC5BTK - SK

NASA astronaut Janice Voss, KC5BTK, of Houston, Texas, passed away on February 7 from cancer. She was 55. One of only six women who have flown in space five times, Voss’ career was highlighted by her work and dedication to scientific payloads and exploration. Voss participated in making ham radio contacts from space via the Space Shuttle Amateur Radio Experiment (SAREX), the precursor to the Amateur Radio on the International Space Station (ARISS) program.

“As the payload commander of two space shuttle missions, Janice was responsible for paving the way for experiments that we now perform on a daily basis on the International Space Station,” said Peggy Whitson, Chief of the Astronaut Office. “By improving the way scientists are able to analyze their data and establishing the experimental methods and hardware necessary to perform these unique experiments, Janice and her crew ensured that our space station would be the site of discoveries that we haven’t even imagined. During the last few years, Janice continued to lead our office’s efforts to provide the best possible procedures to crews operating experiments on the station today. Even more than Janice’s professional contributions, we will miss her positive outlook on the world and her determination to make all things better.”

Voss began her career with NASA in 1973 while a student at Purdue University. She returned to NASA in 1977 to work as an instructor, teaching entry guidance and navigation to space shuttle crews. After completing her PhD in 1987, she worked within the aerospace industry until she was selected as an astronaut in 1990.

Voss’ first spaceflight mission was STS-57 in 1993, the first flight of the SPACEHAB module. She next flew on STS-63 in 1995, a mission to the Mir space station and third flight of SPACEHAB. She also flew as a payload commander on STS-83 in 1997 with the Microgravity Science Laboratory (MSL), but the mission was cut short due to problems with one of the orbiter’s three fuel power generation units. Voss, the crew and MSL flew again as the STS-94 MSL-1 Spacelab mission, which focused on materials and combustion science research in microgravity.

Her last mission was STS-99 in 2000, a flight to the International Space Station (ISS) as part of the Shuttle Radar Topography Mission, which mapped more than 47 million square miles of the Earth’s land surface. In total, Voss spent more than 49 days in space, traveling 18.8 million miles in 779 Earth orbits.

From 2004-2007, Voss served as the science director for the Kepler spacecraft at NASA’s Ames Research Center. Designed to search for Earth-size planets orbiting distant stars, Kepler was launched in March 2009; to date, it has confirmed 61 exoplanets and identified more than 2000 planetary candidates. Voss most recently served as the payloads lead of the Astronaut Office’s Station Branch.

Thanks to NASA , AMSAT and ARRL for the information.

TV News Report on ISS Contacts

This TV news report from 2010 covers the contacts Thomas Medlin W5KUB had with astronaut Doug Wheelock KF5BOC while he was on the International Space Station.

Thomas Medlin W5KUB talked to Doug KF5BOC 29 times while he was commander of the ISS and Tom sent Doug some Memphis BBQ for his first meal after returning from 6 months in space.

Watch the TV news item followed by an interview with Doug who talks about the Memphis BBQ.

W5KUB website http://w5kub.com/

RS-39 (Chibis-M) Deploys

RS-39 Chibis-M

RS-39 Chibis-M

RS-39 has CW beacons on 435.315 and 435.215 MHz that can be received directly by schools and colleges for educational outreach purposes. It deployed from Progress M-13M into a 500 km orbit on January 24 at approximately 23:18:30 UT.

On November 2, 2011 cargo ship “Progress M-13M”, which also delivered microsatellite “Chibis-M”, was docked with ISS. The main purpose of “Chibis-M” is the study of physical processes in the vicinity of the lightning, during which the Terrestrial Gamma Ray Flashes (TGFs) are generated. TGFs are likely produced by beams of very energetic electrons, which are accelerated in the intense electric fields generated by large thunderstorm systems.

The deployment of “Chibis-M” in a circular orbit of 500 km will take place during the final phase of “Progress M-13M” operation. According to the plan of the Russian Space Control Centre, undocking of “Progress M-13M” will occur at January 24, 01:59 msk and after two corrections it will be positioned at 500 km orbit. At January 25, 03:14 msk “Chibis-M” will separate. Beside scientific data “Chibis-M” will transmit service telemetry (the housekeeping parameters) in the beacon format on 435.315 or 435.215 MHz CW (Doppler shift +/- 10 kHz) and has the designation of RS-39. The format of data is typical for RS satellites and can be downloaded here.

The telemetry of RS-39 can be easily received directly by schools and colleges for educational outreach purposes. This telemetry will give details of the spacecraft’s health – battery voltages and temperatures of critical units. In combination with orbital data such information will be useful as the curriculum for student lessons.

The team of RS-39 will very much appreciate any reception reports of “Chibis-M”. Special attention is requested for the first orbits as these are outside of control stations for “Chibis-M”. Each report will be confirmed by special QSL card. The email address is amateur-rs39@chibis.cosmos.ru

The RS-39 Chibis-M website managed the by Space Research Institute of the Russian Academy of Sciences (RAS) can be seen in Russian at http://chibis.cosmos.ru/ or in Google English at http://tinyurl.com/RS-39-Chibis-M

As well as measuring electromagnetic parameters of “space weather” in the spectrum 0.1 – 40 kHz the satellite also carries a receiver for the analysis of radio frequency signals in a frequency band of 26-48 MHz. http://www.energia.ru/en/iss/researches/geophis/19.html

RS-39 Morse Code telemetry format http://tinyurl.com/RS-39-Morse-Code-Telemetry

RS-39 Telemetry Decoder http://www.uk.amsat.org/4029

RS-39 Real Time Tracking Map http://chibis.cosmos.ru/cyclogr/prepare1/google/index.html
For Keps click on two gear wheels in top left-hand corner then click on Satellites.

It may be worth checking the AMSAT Bulletin Board (AMSAT-BB) for the very latest news. The 48-hour archive of the AMSAT-BB is at http://www.amsat.org/amsat/archive/amsat-bb/48hour/threads.html or you can join the bulletin board at http://www.amsat.org/amsat-new/tools/maillist/maillist.php

QRP APRS Packet Radio to the ISS

International Space Station

International Space Station

Doug Cook KD5PDN’s article about contacting the International Space Station with a few watts and a shoestring budget antenna is now available.

The article “QRP to the ISS” appeared in the February, 2012 issue of QST magazine and, with permission from the ARRL, can be downloaded from Clint Bradford K6LCS’s website.

Doug walks the reader through building a simple tape measure beam, and how to successfully work the ISS with it and a handheld radio.

Read the article at http://www.work-sat.com/Work-Sat/Misc_files/QRP-ISS.pdf

A video by author Doug Cook KD5PDN shows the tape rule antenna and how to set up a Yaesu VX-8R for ISS APRS packet data sending and receiving and other aspects to make a digital contact with the International Space Station. You can also learn how to interpret the audio prompts when packet data is being received.

Watch ISS APRS Contact with a Yaesu VX-8R WB5BSA

There is lots of other information on the Work Satellites website at http://www.work-sat.com/

Launch date fixed for Esa's Vega rocket

Europe has named Thursday 9 February as the day it intends to launch its new Vega rocket for the very first time.Vega

The 30m-tall vehicle has been developed to take payloads up to 1.5 tonnes into a polar orbit, and will fly from the Kourou spaceport in French Guiana.

The project has been led by Italian industry and is years behind on its original schedule.

But European Space Agency Director General, Jean-Jacques Dordain, said he would not force the pace.

“Today, the target date is 9 February, but it’s a target,” he told BBC News.

“I shall never say this is the definitive launch date because it is a maiden flight, and with a maiden flight I shall take no risk. There will be no compromise on any question which could still be open on 9 February.”

The caution is well advised. Statistics show that some two-thirds of the rockets introduced in the past 20 years have had an unsuccessful first outing.

It is for this reason that the satellites carried on the “qualification” flight have been given a free ride.

Biannual operations

Vega is a four-stage rocket. Its first three segments burn a solid fuel; its fourth and final stage uses liquid propellants, and can be stopped and restarted several times to get a spacecraft into just the right orbit.

Esa expects an operational Vega to be launching about twice a year, carrying mostly small scientific and government satellites.

If the rocket should need to delay from 9 February to deal with technical issues, it will only be given a short window to resolve the problems before being asked to stand down for several weeks.

Vega’s big “brother” at Kourou, the Ariane 5 rocket, is booked to launch Europe’s third ATV cargo ship to the International Space Station (ISS) on 9 March, and this mission will take precedence if there is a conflict.

The frequent comings and goings at the orbiting platform require a carefully co-ordinated traffic schedule, and this will not be disrupted for an unrelated, experimental rocket flight.

“I have to respect my commitments to my International Space Station partners,” Mr Dordain explained.

“It’s clear that if we are arriving in a situation where the launch of Vega starts to interfere with the date of the launch of ATV 3, I will choose to switch and go for ATV first and Vega next.”

Long-term planning

Vega is just the beginning of what is expected to be a busy year for Esa.

Metop-BMetop-B will launch in May/June

Other highlights include the launch of two major weather satellites, Meteosat 10 and Metop-B, and a trio of craft called Swarm that will measure the Earth’s magnetism in unprecedented detail.

Policy-wise, 2012 will also be a significant year because it will see the first Ministerial Council since 2008. This gathering of the member states, to take place in Italy in November, will set programmes and budgets for the next three to five years.

Key decisions will need to be made on the next evolution of Ariane, on funding for Esa’s participation in the ISS project, and on the development of a next-generation of polar orbiting weather satellites to succeed the Metop series.

Nations are likely to go to the meeting in a much weaker position economically than they did in 2008.

Nonetheless, Mr Dordain expressed satisfaction with Esa’s current budget profile.

The agency will have essentially a flat income this year of 4.02bn euros (£3.32bn), when all contributions, including from the EU, are taken into account).

“I am trying to implement the Esa programmes with just the payments that are necessary – less and less margin, more and more efficiency, and more and more reduction of internal costs,” Mr Dordain said. “This is a daily challenge, but on the other hand it makes life interesting.”

Germany and France continue to be the lead contributors to Esa, although it is noteworthy that the former’s agency contribution now exceeds that of the latter (750m euros from Germany versus 717m euros from France). Italy (350m euros) and the UK (260m euros/£215m) make up the rest of the “big four”.

Jonathan.Amos-INTERNET@bbc.co.uk

Launch date fixed for Esa’s Vega rocket

Europe has named Thursday 9 February as the day it intends to launch its new Vega rocket for the very first time.Vega

The 30m-tall vehicle has been developed to take payloads up to 1.5 tonnes into a polar orbit, and will fly from the Kourou spaceport in French Guiana.

The project has been led by Italian industry and is years behind on its original schedule.

But European Space Agency Director General, Jean-Jacques Dordain, said he would not force the pace.

“Today, the target date is 9 February, but it’s a target,” he told BBC News.

“I shall never say this is the definitive launch date because it is a maiden flight, and with a maiden flight I shall take no risk. There will be no compromise on any question which could still be open on 9 February.”

The caution is well advised. Statistics show that some two-thirds of the rockets introduced in the past 20 years have had an unsuccessful first outing.

It is for this reason that the satellites carried on the “qualification” flight have been given a free ride.

Biannual operations

Vega is a four-stage rocket. Its first three segments burn a solid fuel; its fourth and final stage uses liquid propellants, and can be stopped and restarted several times to get a spacecraft into just the right orbit.

Esa expects an operational Vega to be launching about twice a year, carrying mostly small scientific and government satellites.

If the rocket should need to delay from 9 February to deal with technical issues, it will only be given a short window to resolve the problems before being asked to stand down for several weeks.

Vega’s big “brother” at Kourou, the Ariane 5 rocket, is booked to launch Europe’s third ATV cargo ship to the International Space Station (ISS) on 9 March, and this mission will take precedence if there is a conflict.

The frequent comings and goings at the orbiting platform require a carefully co-ordinated traffic schedule, and this will not be disrupted for an unrelated, experimental rocket flight.

“I have to respect my commitments to my International Space Station partners,” Mr Dordain explained.

“It’s clear that if we are arriving in a situation where the launch of Vega starts to interfere with the date of the launch of ATV 3, I will choose to switch and go for ATV first and Vega next.”

Long-term planning

Vega is just the beginning of what is expected to be a busy year for Esa.

Metop-BMetop-B will launch in May/June

Other highlights include the launch of two major weather satellites, Meteosat 10 and Metop-B, and a trio of craft called Swarm that will measure the Earth’s magnetism in unprecedented detail.

Policy-wise, 2012 will also be a significant year because it will see the first Ministerial Council since 2008. This gathering of the member states, to take place in Italy in November, will set programmes and budgets for the next three to five years.

Key decisions will need to be made on the next evolution of Ariane, on funding for Esa’s participation in the ISS project, and on the development of a next-generation of polar orbiting weather satellites to succeed the Metop series.

Nations are likely to go to the meeting in a much weaker position economically than they did in 2008.

Nonetheless, Mr Dordain expressed satisfaction with Esa’s current budget profile.

The agency will have essentially a flat income this year of 4.02bn euros (£3.32bn), when all contributions, including from the EU, are taken into account).

“I am trying to implement the Esa programmes with just the payments that are necessary – less and less margin, more and more efficiency, and more and more reduction of internal costs,” Mr Dordain said. “This is a daily challenge, but on the other hand it makes life interesting.”

Germany and France continue to be the lead contributors to Esa, although it is noteworthy that the former’s agency contribution now exceeds that of the latter (750m euros from Germany versus 717m euros from France). Italy (350m euros) and the UK (260m euros/£215m) make up the rest of the “big four”.

Jonathan.Amos-INTERNET@bbc.co.uk