Author: Pradeep

  • Changing Mumbai in places where I walk

    Note: I wrote this on my earlier blog hosted as https://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on March 14, 2011 as per the permalink. I’m trying to collect here again all my old writings spread on various blogs.

    I have made it a practice of going on early morning walks (if my father wakes me up). It used to painful in the early days which surprised me given the amount of walking I already did. Dad set a new understanding of what it means to walk quickly. I took my time getting accustomed to faster walking. Friends have always complained that I walk fast. In the mornings, I walk faster. Those early days of pain made me not want to walk again in the evening. Habit set in and I slowly lost my evening walking fun.

    In the last two days, I have started the evening walk routine again. This slower walking is for me to notice the changes around my suburb of Chembur. Hit by projects like the Monorail and the Chembur-Santacruz Link Road projects, the places that I walk in is transforming at a very fast pace. Now, I feel that I have lost something of the memories by not photographing it.

    The construction work in these lanes has transformed the once sleepy lanes into a very different experience. Walking down these roads is less fun now. I don’t know how it would be after the roads and monorail are built. Some one has to chronicle this history of a metamorphosing metropolis. Once sleepy lanes that I used to haunt could in the near future become crowded monorail stations or metro stops. Nostalgia is slowly walking in and I am looking for other sleepy lanes to haunt.

  • Trek to Korlai Fort

    Note: I wrote this on my earlier blog hosted as https://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on March 14, 2011 as per the permalink. I’m trying to collect here again all my old writings spread on various blogs. The original post had a gallery of pics, I have replaced that with one representative picture.

    In January, I finally got my membership for the Youth Hostels Association of India for two years. I was looking out for a way to utilise the membership but no opportunity presented itself till March 6, 2011 when the Mumbai unit went on a trek to Korlai Fort. It has been a long time since I went trekking and I did not want to do a trek labelled “hard” by the trekkers themselves. I therefore chose a “medium” trek.

    I learnt from Ganesh that they were travelling by ST bus and that I could come along. I immediately flagged it to Pranav’s attention. After a few rounds of conversation, I decided to head down to Parel ST Bus Depot while Pranav decided to catch up with us at Korlai on the next day. I packed a bag that was just heavy and was filled with stuff I never would have used. I packed a 1.5 liter water bottle and managed to alternately over-hydrate and under-hydrate myself. Well, I am happy that it was a simple enough trek so I didn’t have to think about too many things at the same time. There also seemed to be a malfunction in my camera’s battery indicator which showed that the battery was full when it was really drained. I read up about Korlai Fort on Wikipedia and found out that the article on Korlai itself was speedily deleted by someone.

    Dad insisted on dropping me at Parel ST Stand which is very oddly situated. It was because I informed the YHAI guys only on the previous day that I had to travel there. Else, I could think about joining them at Chembur. The ST depots in Maharashtra are not as good as the ones in Kerala or Tamil Nadu but are much better than my last experience of them. The buses were more of a surprise for me. The travel was particularily smooth and the journey was particularly pleasant. We had wada pav at Alibaug and then proceeded to Revdanda and then crossed the river to Korlai reaching the bus stop at 10:30 in the morning. We then walked through the small village of Korlai as we headed towards the hill on which the fort was built.

    We per-ordered lunch at a small hotel before the climb and then walked through open pans were fish were left to dry and walked up a tar path to the base of the hill. We then rested a bit at the bottom and then walked up the road that went along a side of the fort. The road had a small beach to one side and the hill slope on the other. Ahead we saw the Korlai Fort Lighthouse. A manager at the gate offered a paid tour of the interior of the lighthouse. We had to pay extra to take pictures. I thought it wise to conserve battery (and by now I got the hang of Pranav’s insatiable desire for getting himself photographed). I like the scenery a bit more. Hence, I passed by the offer and went to take a look inside the light house.

    The manager explained that the lighthouse was automated and it pretty much took care of itself. The workers on site were mostly there to do maintenance work and to check the instrumentation once or twice a day. We passed through two narrow holes in the ceiling to reach the top of the light house. The manager explained how the lighthouse worked, how it was now mostly used by fishermen more than anyone else and the presence of modern technology stuff like transmitters and satellite dishes that one really did not see in a lighthouse. The structure did not need to be big because of the kind of boats it helped. It helped fishermen go deeper into the sea and get better and a variety of catch. There were even solar panels that charged the battery during the day for when there would be power cuts.

    We left the manager and climbed a steep set of steps to the fort. I took quite a few number of breaks in between. Learnt that pacing yourself isn’t as easy as saying, “You have to pace yourself.” After walking around the fort, we left out through the other gate. I also felt the afternoon high sun taking a toll on me and then had a hard time getting to the base of the hill. We steadily went down one of the wings of the fortress that touched the sea and then had a round of introductions and took group photos. We then went to the side in through a nice tunnel with a pleasant breeze and sat for a while. We began the slow ascent, a walk through the main corridor and reached the main fort area.

    We’d heard of a water source that was fresh inside of the fortress and we were interested in tasting some. We also had group members discuss the history of the fort and we had a nice time chatting about the forts of the Siddis known to have resided in the area of Alibaug during the reign of Shivaji and Sambhaji. We saw a temple and a broken down church and signs of the restoration work that was being carried out by Archaeological Survey of India. There were many cement packs in the fort and we joked that these were uncovered along with the rest of the fort. The water in that natural tank was quite good and very refreshing after that long ascent.

    We had lunch at the hotel where we had pre-ordered the food and took a big auto all the way back to Alibaug. I hung around on the beach as the rest of the group went to visit Alibaug Fort. On the beach, the others got to leave their bags and I got to have a gola which I’ve not had in a very long time. I had a fun time just resting without the hiking shoes and even though the early evening sun was hot, the sitting down helped a lot.

    After the others returned, we walked back to the Alibaug ST bus stand and from there, we headed back home in a ST bus. The driver was happy enough to let us sleep and switch off the lights. At night I was not able to see the roads and didn’t understand much of the route until we reached Panvel at night. A bit of a heavy dinner at night meant that I got sound sleep.

  • Indian Perspectives on Human Spaceflight

    Dr. Harish, Deputy Project Director, Human Spaceflight Programme, ISRO spoke at Aero India 2011 held recently in Bangalore. The title of this article made me excited enough to want to watch it.

    However, after watching the video, it was quite general. His talk was very non-specific and did not have much matter. Some points though involved the choice of the Soyuz style architecture for the crew vehicle based on the Shuttle vs Soyuz experience and safety record of the US and Russia respectively. He talked about how humans would control the flight very mysteriously without expanding on it. He explained that the experience with the Space Capsule Re-entry Experiment (SRE) gave ISRO the confidence to go ahead with the human spaceflight programme. He put across that putting an air conditioning on the SRE would give us the crew vehicle – which is a rather crude way of putting it. He talked about how experience of Apollo management style has influenced India and last but not the least he explained that there is excessive stress on safety.

    I do not think that a keen follower of the programme would have missed anything if he did not listen to this talk. However, if you have the time or the inclination, feel free to go through the video. I would like to stress again that Indian scientists and engineers need to get much better at communicating to the common man what they’re doing.

  • Reason for the Long Solar Minimum

    Note: I wrote this on my earlier blog hosted as https://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on March 03, 2011 as per the permalink. I’m trying to collect here again all my old writings spread on various blogs.

    A project funded by the National Aeronautics and Space Administration (NASA) and Department of Science and Technology (DST) of the Government of India has claimed to have found the reason for the long solar minimum experienced during the last solar cycle. A team led by Indian Dibyendu Nandy of the Indian Institute of Science Education and Research (IISER), Kolkata which included Andrés Muñoz-Jaramillo of Montana State University and Petrus C. H. Martens of the Harvard-Smithsonian Center of Astrophysics.

    The results will be presented in Nature magazine today. Nandy has made this webpage about the discovery which to me is incomprehensible. My friend Srinivas Laxman wrote this article in today’s Times of India which fares a bit better for comprehension sake. For me the best article on the discovery was by Dr. Tony Philips writing for NASA Science News.

    NASA held a media tele-conference on the topic and hence this was widely covered by the press in the US. There seems to be little to no press coverage of the topic in India besides the one written up by Srinivas Laxman.

  • Budgetary Allocation for the Department of Space in Budget 2011-12

    If you have the time, I request you to consider reading the document in full (Excel Sheet). If you do not, here is the document with planned budgetary allocation for 2010-11 against revised figures  in 2010-11 in crores of Rupees:

    • Development of the GSLV Mk-III:  125.64 (against 130.78)
    • Cryogenic Upper Stage Project: 0.1 (against 0.1)
    • Continuation of the PSLV: 244.50 (against 224)
    • for the Vikram Sarabhai Space Center: 463.03 (against 375.18)
    • for the ISRO Intertial Systems Unit: 39.74 (against 29.63)
    • for the Liquid Propulsion Systems Center: 231.33 (against 203.02)
    • for the GSLV (including the Mk-III): 292.46 (against 209.10)
    • Space Capsule Recovery Experiment: 4.40 (against 4.79)
    • Manned Mission Initiatives/Human Space Flight: 98.81 (against 14.71)
    • Indian Institute of Space Science and Technology: 100 (against 10)
    • Semi-Cryogenic Engine Development: 150 (against 40)
    • Oceansat-2 and -3: 50 (against 10)
    • Resourcesat-2 and -3: 32.66 (against 22)
    • ISRO Satellite Center: 233 (against 244.60)
    • Laboratory for Electro-Optical Systems: 42.85 (against 36.71)
    • RISAT-1: 0.95 (against 2)
    • GSAT-4/GSAT-4R/GSAT-11EM: 50 (against 0)
    • Navigation Satellite System:  218.30 (against 167.40)
    • Semi-Conductor Laboratory: 45.72 (against 26.42)
    • Advanced Communication Satellite (including GSAT-11): 410 (against 35)
    • Earth Observation – New Missions, (Cartostat-3, TES Hyperspectral, DMSAR-1,ENVISAT,SCATSAT,RISAT-3, Future EO Missions and GISAT): 200 (against 0)
    • SARAL: 22.5 (against 13)
    • Satish Dhawan Space Center: 337.25 (against 261.51)
    • ISTRAC: 45.75 (against 53.75)
    • Space Applications Center:  291.99 (against 183.80)
    • Development and Education Communication Unit: 73.56 (against 22.76)
    • National Natural Resources Management System: 72.84 (against 42.06)
    • Earth Observation Application Mission: 2.53 (against 2.33)
    • National Remote Sensing Center: 145.55 (against 154.49)
    • Disaster Management Support: 34.57 (against 29.97)
    • North Eastern Space Applications Center: 6.07 (against 0)
    • Physical Research Laboratory:  48.31 (Against 33.97)
    • National Atmospheric Research Laboratory: 16.44 (against 8.43)
    • National Institute of Climate Change and Environmental Studies: 0.1 (against 0.1)
    • RESPOND: 15 (against 14)
    • Sensor Payload Development/Planetary Sciences Programme: 30 (against 8.25)
    • Megha-Tropiques: 2 (against 10)
    • ADITYA: 40 (Against 5.75)
    • ASTROSAT-1 and -2: 10 (against 10)
    • Chandrayaan-1 and -2: 80 (against 25)
  • Talk by R Navalgund

    Note: I wrote this on my earlier blog hosted as https://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on March 01, 2011. I’m trying to collect here again all my old writings spread on various blogs.

    I went to the Tata Institute of Fundamental Research (TIFR) on Monday to hear the National Science Day Public Lecture organised by TIFR and the TIFR Alumni Association. The talk was delivered by Ragunath Navalgund, Director, Space Applications Center, Indian Space Research Organisation (ISRO).

    At the welcoming address, the TIFR Director gave us a brief about how the day, February 28 had come to being celebrated as National Science Day. He said it was the day that C V Raman had submitted the manuscript which talked about the Raman Effect for the first time. The discovery of the Effect gave Raman a Nobel Prize and is still one of the most renowned discovery by an Indian scientist. He said further that Raman used to give public talks on science in a manner which was understandable to the general public. This is perhaps one of the first examples of science outreach by an Indian scientist. The day was later adopted by the Government of India to be called National Science Day. At TIFR, the day was celebrated by lectures from prominent alumni members.

    R Navalgund then gave the Director a copy of the lunar atlas with pictures from the Chandrayaan-I spacecraft. I was thinking of nicking it!

    Navalgund began his talk titled, “Remote Sensing of the Earth and the Moon” by talking about remote sensing in general. He defined it and explained how it was different from “seeing with our eyes”. He explained the difference as being sensing in various wavelengths of the electromagnetic spectrum other than just visible light like our eyes. The results are in the form of data sets which are then converted into images. He explained that remote sensing was done from various platforms – low-Earth orbit and geo-stationary orbits depending on their applications.

    He moved on to various types of sensing – active and passive and then explained the various techniques of remote sensing. He showed the push-broom type, the pixel-by-pixel type, the synthetic aperture radar and the hyperspectral imaging.

    He talked about how various parts of the electromagnetic spectrum could be studied in individual bands interacted with objects on the ground and how these could help in providing useful information. As an example, he talked about studying leaves with red light and near infra red light to understand if leaves were healthy or mature. This data helped in providing the Government a plausible estimate of the healthy plants in the country well before the harvesting period. Similar studies were done in various spectrum for hydrology, cryosphere, forest cover, atmosphere and oceans to provide similar information. Information involved ground water levels, forest covers, smogs, possible fishing zones, crop health prediction and yield.

    He then moved on to the remote sensing of the Moon. He showed the various types of craters and features like the central peaks of craters and impact melts. He also showed pictures from the recently discovered lava tube.

    The interesting points though came out in the question and answer session. Answering questions by students from Kendriya Vidyalaya, Navalgund came out with quite a few interesting points that were unknown. Speaking on India’s participation in the International Space Station (ISS), he said that there was an informal agreement on the possibility of India conducting experiments on the ISS. He said that the discussions were currently on in this regard. The experiments, he said, would relate to the study of green house gases. He said Indian institutions would have to provide a proposal for these experiments and some would also come from within ISRO. Answering another question on the Human Spaceflight Programme, he said that all the designs, approvals and paper work was done. The Programme had got an in-principle nod from the Indian cabinet. Discussions were currently on as to how to implement the programme. The two ideas included doing the testing in a single shot or testing the elements individually as done with Space Re-entry Experiment (SRE). He said the programme was in this phase currently. Answering a question I posed, he shocked me by saying that data from the Terrain Mapping Camera (TMC) and Hyper Spectral Imager (HySI) have been made available online. Srinivas found the website for me, it is here. Navalgund explained that the images were released only after 1 year to aid the investigations done by principal investigators who were the primary users of the data. He said that NASA had separately released the data from the Moon Mineralogy Mapper (M3). On Mars, Navalgund said that the plans were currently in drawing board phase and currently, India only had capability to do a flyby or orbiter programme indigenously.

    My friend, Srinivas asked the question about why India’s CHACE instrument was not given the credit for the lunar water discovery as much as M3 or even Mini-SAR. Navalgund replied that the instrument did have a short operation span and did find spectrum peaks for water, carbon dioxide and other elements. He said a lot of time was spent on calibrating the data properly. This was a long drawn process which possibly led to the CHACE losing out on the credit for the water discovery.

    I also met a member of the newly joined Google Lunar X Prize team, Team Indus at the lecture.

  • Using Chandrayaan-I to find human habitability sites on the Moon

    Note: I wrote this on my earlier blog hosted as http://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on February 24, 2011 as per the time stamp. I’m trying to collect here again all my old writings spread on various blogs.

    The current edition of Current Science magazine has the paper by Arya et. all titled, “Detection of potential site for future human habitability on the Moon using Chandrayaan-1 data“. The result itself was reported way back in March, 2010. The paper provides more details and some interesting facets. The paper is based on work done by the Terrain Mapping Camera on board the Chandrayaan-I spacecraft.

    The high spatial resolution of the Terrain Mapping Camera and the close 100 km orbit helped scientists build Digital Elevation Models (DEM) to help study the lunar terrain in great detail. This was used to study potential human habitability sites on the Moon. Based on previous studies, they concentrated their efforts on riles and lava tubes on the lunar surface. Study on the Oceanus Procellurum region on the Moon showed that lava tubes were good places for possible human habitability. They found that there was no effect of cosmic rays deeper than 6 meters, no effect of solar particles deeper than 1 meter, no radiation effects and no significant temperature difference was observed with the temperature remaining nearly constant at -20 degrees Celsius. It is also opined that the presence of partial lava tube structure reduces requirement of construction. Scientists also think that the cool temperatures here could make these a candidate for water and ice traps on the lunar surface. Lava tubes also provide a dust free environment.

    Lava Tubes are interesting to study for reasons other than human habitability as well. To geologists, it provides a section of the lunar bedrock and top soil that would be difficult to access otherwise. It could also help geologists to study native lunar material which has not been affected by external factors like meteoric impacts, solar particles etc. It could also provide an understanding of the thermal profiles and volcanism on the Moon.

    The paper now profiles the area of the Moon under study, Oceanus Procellurum using a picture of the Moon taken by the CARTOSAT-2A spacecraft from Earth orbit!

    Using various techniques (explained in the paper) they find that the rough cylindrical tube which comprises the lava tube is 120 meters in diameter and 1.72 km in length. The thickness of the roof is 170 meters hence safe from various considerations discussed above (radiation, cosmic rays etc.). The Hyper Spectral Imager (HySI) was used to do chemical and mineralogical study. It was found that the surface was homogeneously basaltic rich in Iron and Titanium. The homogeneity of  the results was also used to predict that there was no lava flow after the lava tube was formed. To confirm the result, surface ages of the north and south section of the uncollapsed rille was done using the crater counting technique. Using this method ages of the northern section was found to be 3.47 Ga and the southern section was found to be 3.43 Ga. This more or less rules out “differential emplacements of the mare basalts”.

    The authors of the paper state that using similar procedures, TMC and HySI data can be used to study different areas on the surface of the Moon.

  • Three Chandrayaan-I related papers out

    Note: I wrote this on my earlier blog hosted as http://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on February 23, 2011 as per the time stamp. I’m trying to collect here again all my old writings spread on various blogs.

    Three papers directly related to instruments on-board the Chandrayaan-I spacecraft are out in 2011. Here’s a brief pointer to each.

    1. Goldschmidt crater and the Moon’s north polar region: Results from the Moon Mineralogy Mapper (M3); Cheek, Pieters et. all

    2. Strong influence of lunar crustal fields on the solar wind flow [full paper – PDF]; Charles Lue et. all

    3. Lithological mapping of central part of Mare Moscoviense using Chandrayaan-I Hyperspectral Imager (HySI) data; S Bhattacharya et. all

    For the first paper, Cheek et. all, have trained their eyes on the Goldschmidt crater. The comparison of spectroscopic details from Goldschmidt to the Moon Mineralogy Mapper (M3)’s data of the Northern pole and from three different regions provide three different soil types – feldspathic soils with a low-Ca pyroxene component, feldspathic soils and basaltic soils. The content of Goldschmidt is feldspathic and was found to be locally different from the surrounding highlands. They state that the water spectrum is closely associated with the mineralogy of where the spectrum is located. Goldschmidt is said to have higher concentration of water spectrum compared to the local highlands but is similar to the feldspathic soil in the lunar far side.

    The second paper by Charles Lue et all is available in full. The SARA payload on Chandrayaan-I had detected the presence of mini-magnetospheres on the surface of the Moon. The paper Lue et. all believes that these magnetospheres affect the upstream solar winds. This affect the rate of solar wind proton hitting the surface of the Moon and also perhaps space weathering in places near the magnetic anomalies. The team uses data from the Solar Wind Monitor (SWIM) on Chandrayaan-I for these studies. Concluding, they say:

    Magnetized electrons are deflected by the magnetic field gradient and set up a charge separation (because  protons are non‐magnetized), resulting in an ambipolar  electric field. The related potential repels a fraction of the  protons. Therefore, the deflection can take place not only  over the strongest magnetic anomalies where the protons can  be magnetized, but (although at a lower efficiency) also at  weak, isolated anomalies of ❤ nT at 30 km altitude, with a  width of <100 km. Similar charge separation scenarios have  been discussed in early studies based on Apollo 12 surface  observations [e.g., Neugebauer et al., 1972], and in a recent  review paper by Halekas et al. [2010].

    This paper too has some influence on the lunar water formation technique suggested of solar wind implanting protons which are used by the OH ions to form water:

    Regardless of the deflection mechanism for protons,  the high solar wind deflection and reflection rates, as ions  and neutral atoms, imply a lower proton implantation rate in  the regolith at magnetic anomalies that may alter the space  weathering compared to the surrounding areas. Moreover, it  might affect the production of OH/H2O in the outermost  layer of the regolith via transfer of solar wind‐implanted  protons to the mineral‐bound oxygen [Pieters et al., 2009].

    The paper is available here in full.

    The third paper, Bhattacharya et all investigated the central region of the Mare Moscoviense region of the Moon. The paper has identified 5 geological units:

    five major compositional units have been identified: highland basin soils, ancient mature mare, highland contaminated mare, buried unit with abundant low-Ca pyroxene (LCP), and youngest mare unit

    The paper seems to be aimed as basis of using the Hyper Spectral Imager (HySI) data to delineate major compositional structures on the surface of the Moon and has done so successfully enabling it to be used for the rest of the data sets obtained.

  • Madhavan Nair’s comments in the Media

    Note: I wrote this on my earlier blog hosted as http://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on February 22, 2011 as per the time stamp. I’m trying to collect here again all my old writings spread on various blogs.

    Madhavan Nair has recently been on a commenting and interviewing spree. The bulk of his effort seems to be deflect blame from ISRO on two recent events – the failure of the GSLV and the ISRO/DEVAS deal. His comments on the failure of the GSLV seem a little out of line. His comments on the ISRO/DEVAS deal could be considered as an effort to deflect blame from himself. Whatever the case, his media interactions since the GSLV failure has been interesting to follow.

    I have never seen a chair of any failure analysis committee commenting on the progress of the committee as the analysis was on-going. Madhavan Nair seems to be repeating the same statement since the first meeting held in January. He’d begun pointing to the Russian cryogenic engine for the failure of the GSLV in December. This changed from the “German connectors” blamed initially for the failure. The interesting point about this repeated statement is that while Russia is willing to “studying the data provided to them”, Madhavan Nair seems to be stressing on this point. Also, ISRO seems to be conducting experiments and we’re running dangerously close to the last date for the submission of the report of the GSLV Failure Analysis Committee under the chairmanship of Madhavan Nair. I would think a meeting would be needed to get the results, analyse them and create a cohesive report. Madhavan Nair’s various comments [see here and here] to the media vis-a-vis the GSLV seems to be beyond the control of ISRO.

    His other interesting comment comes on ISRO/DEVAS issue. I have refrained from commenting on the issue here since my understanding of the same has been very poor. Madhavan Nair did an interview with the Times of India on the issue. His version of the story matches more closely with the version put out by DEVAS than by ISRO. This has now pushed the Opposition to demand that the Prime Minister (who’s in-charge of the Department of Space) to make a statement in Parliament on the issue. Madhavan Nair’s comments carry weight because he was the man in-charge in ISRO when the deal was operationalised. It seems like Nair is trying to protect himself. It even seems to have worked partially since the Opposition has turned its attention again from him.

    While on the topic of ISRO/DEVAS, I’d also like to point out the different approaches that ISRO and DEVAS have taken to put out their statements. ISRO has put out a 5 page PDF (now removed!!) that is a bit confusing and leaves a few questions un-answered and DEVAS has posted a video in a FAQ format that lasts about 4 minutes.

  • Public Lecture by Sir Arnold Wolfendale

    Note: I wrote this on my earlier blog hosted as http://parallelspirals.blogspot.com. I recovered the text from the WayBack Machine. This post appeared on February 21, 2011 as per the time stamp. I’m trying to collect here again all my old writings spread on various blogs.

    Sir Arnold Wolfendale gave a public lecture at the Marathi Vignan Parishad offices located in Chunabhatti. I saw this place for the first time when I was in a bus and was stuck in the famous Priyadarshini traffic jam. I was interested in going to this place but like everything else never got around to going there. My friend, Suhas Naik-Sattam who works at the Nehru Planetarium informed me about the event through Facebook. The talk was easy to understand and punctuated by humour and his experience over the years.

    The talk was a collaboration between National Centre for Science Communicators, Marathi Vignan Parishad, Khagol Mandal and International Union of Science Communicators. The talk was titled, “Search for Extra Terrestrial Intelligence”. Before beginning, he took a straw pole of the number of people who believed that we were alone in the Universe (or unique) and the number of people who thought we were not. Only 11 people in the whole room said that we were a unique species in the Universe. Rest of the audience, probably numbering about a 100 with school children involved said that we were not alone. Wolfendale said that over the years, when the same question was asked of the audience only 27% of the audience said that we were a common species.

    Wolfendale then shared a story. He said a scientist retired and got himself a place at one of the places in England which end up with a sheer cliff and jagged rocks at the bottom of the cliff and the sea beneath. Once, exploring the stars, the man tripped over and by chance got hold of a branch on the drop. He called for help when a heavenly voice asked him to let go and that He would catch him. “Anybody else, out there?” asked the scientist. Wolfendale said he was looking for that anybody else too – not God.

    He showed a picture of Jodrell Bank’s Lovell Telescope to demonstrate what a radio telescope looked like and then showed the Arecibo and explained how it was used to search for the above mentioned intelligence – life like us – was done from Arecibo. He spoke about expressions of people over the centuries from 13th century Chinese philosopher Teng Mu through Giordano Bruno and Copernicus and Galileo right upto the Kepler looking for planets in the Universe and wondering about the possibility of life on them.

    He then showed the famous Drake Equation, a formula thought to predict the number of detectable civilizations in the Universe. He explained the various terms in the equation, spoke about the possibility of finding their values so that one could substitute them in the Equation to find a plausible result. In explaining these terms, he spoke of SETI and the search started in 1960 by Francis Drake to find the value for “the fraction of civilizations that develop a technology that releases detectable signs of their existence into space”. He spoke of the Mars meteorite activity and how it influenced the debate on “the length of time for which such civilizations release detectable signals into space”.

    Wolfendale postulated possible time frames for which human like life form could evolve and exist. He guessed the number as 1 billion years. He spoke of solar flares that could damage the atmosphere occuring about once in a million years, an asteroid event like the dinosaurs once every 109 years and the life term of the Sun itself being about 4 billion years.

    As he explained this, he gave the evolutionary timeframe and also explained about the rarity of an asteroid impact at Yucatan.

    In the end, he said, if an alien civilization existed and one became extinct every billion years, we should be faced with a barrage of alien colonisations which was not happening and hence he sided with the 11 who said that we were a unique alien life form.

    To me, the ending was an odd bit of reasoning and the talk ended quite suddenly. I did enjoy the initial part of the lecture, though.