It’s been a pretty exciting week to be an asteroid researcher: you’d think the sky was falling! Really, it was just a confluence of some rowdy neighbors checking in on earth asking, “How’s that space program coming?” An ordinary chondrite meteorite exploded over Russia, and later that day a 150-foot-wide piece of spacerock skimmed 17,000 miles above the earth, just ducking inside the orbits of geostationary satellites.
We had nothing to do with either: the Russia bolide was detected maybe seconds beforehand by some satellites; 2012 DA14 was too low in our sky for Arecibo to observe.
The media guy here is still getting calls, almost a week later. Univision came by, Dish Network wanted to interview someone…
What are we doing in the midst of all this? Regularly scheduled observations of asteroid (99942) Apophis, everyone’s favorite potentially hazardous asteroid that we’ve known about for almost nine years now. None of these recently discovered raucous interlopers for us this week, pshaw. Even so, the events of last week underscore the importance of “finding them before they find us” and commercial solutions to asteroid problems.
I spent last week observing of asteroids from the telescope: our first night was just another 8-4 work
day night, where we looked at space rocks in our neighborhood and out beyond Mars for eight hours.
Arriving at the control room, I sat down with my binder full of… notes on how to observe at Arecibo, which hadn’t made much sense. At any optical observatory you enter your coördinates into a computer and take an image. After verifying that you pointed the telescope correctly, you then tell the telescope system to take data for the rest of the night, occasionally adjusting pointing or focus.
At Arecibo, you’re pointed in the right direction. Alignment with the William E. Gordon Telescope is not an issue. Even with the 305-meter dish, you’re good to a few millimeters.
Getting the signal out of the receiver and properly into the computer is the hard part of observing. Instead of a few shiny silvered mirrors and a charge coupled device digitizing and sending your photons to a screen, here a maze of waveguides, cables, and wires brings signals from the matte metal dish, after being ushered into the receivers, along a path 1,600′ long to the control room. Where computer monitors would display starfields at an optical observatory, wavy lines danced across oscilloscopes at Arecibo. It felt like junior year electronics laboratory again in the physics department, so different from most of the things we were doing in astronomy, and not just because of cgs/MKS units arguments.
Ellen had considered walking me through cabling the week before our six-night-long marathon observing run, but ultimately decided that it wouldn’t make sense out of context. Wait for the actual observing run to understand the cabling.
A little over a week ago I arrived at the largest single-dish radio telescope in the world. My boss picked me up at the airport and drove me up into the hills of Puerto Rico’s karst country where I caught my first glimpse of the support towers of Arecibo Observatory, peeking out over the wooded hills.
February 15, 2012
Another year, another telescope trained on another asteroid. I spent the evening of February 15 at the summit of Mt. Hamilton near San Jose with the 40″ Nickel telescope pointed at (22) Kalliope and its moon Linus. The asteroid slowly plodded across the camera frame as the hours ticked by from sunset until 1 am. The weather was clear, if windy. Most of the observing was supposed to be done remotely from a basement at UC Berkeley, but I had to be checked out first at the actual telescope before I could remotely observe, so away I drove to Mount Hamilton.